Difference: DataLog (1 vs. 122)

Revision 1222015-05-20 - boeglinw

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 22 to 22
  Figure Set 3: PD Offsets from RP

Figure Set 4: Detector Angular Orientations

Added:
>
>		 shot_list.data: Shot list
 

Plasma Scenarios

Line: 410 to 412
 
META FILEATTACHMENT attachment="Radial_offset2_scaledlabeled_2.png" attr="h" comment="" date="1392144893" name="Radial_offset2_scaledlabeled_2.png" path="Radial_offset2_scaledlabeled_2.png" size="155181" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_geometry.pdf" attr="h" comment="" date="1392153770" name="detector_geometry.pdf" path="detector_geometry.pdf" size="52093" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_geometry1.png" attr="h" comment="" date="1392153916" name="detector_geometry1.png" path="detector_geometry1.png" size="73423" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="shot_list.data" attr="" comment="Shot list" date="1432142514" name="shot_list.data" path="shot_list.data" size="13678" user="boeglinw" version="1"

Revision 1212014-12-28 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 260 to 260
 
30082 09/06/2013

30082_0.5_0.data

30082_0.5_1.data

30082_0.5_2.data

30082_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
30084 09/06/2013

30084_0.5_0.data

30084_0.5_1.data

30084_0.5_2.data

30084_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
30085 09/06/2013

30085_0.5_0.data

30085_0.5_1.data

30085_0.5_2.data

30085_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
Changed:
<
<
30086 09/06/2013

30086_0.5_0.data

30086_0.5_1.data

30086_0.5_2.data

30086_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: no usable data  
>
>
30086 09/06/2013

30086_0.5_0.data

30086_0.5_1.data

30086_0.5_2.data

30086_0.5_3.data

Carlos Lopez

redone: Ramona Perez

 Yes Yes Yes Yes

Ch 0: no usable data

Ch 0: very noisy, but some peaks

  
 
30087                  
30088                  
30089                  
Changed:
<
<
30090                  
>
>
30090  

30090_0.7_0.data

30090_0.7_1.data

30090_0.7_2.data

30090_0.7_3.data

 Ramona Perez Yes Yes Yes Yes Ch0: very noisy, but some peaks  
 
30091                  
30092                  
30093                  

Revision 1202014-09-10 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 120 to 120
 
29895                  
29896                  
29897                  
Deleted:
<
<
29898                  
 
29899 08/20/13   Douglas No No No No All channels only noise.  
29901 08/20/13   Douglas No No No No All channels only noise.  
29902 08/20/13   Douglas No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.  

Revision 1192014-09-09 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 60 to 60
  Yes
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes  
Changed:
<
<
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes        
>
>
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes        
 
29807                  
29808                  
29809                  
Line: 105 to 105
 
29876                  
29877                  
29878                  
Changed:
<
<
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes    
29880 08/19/13   Werner/ Ramona Yes No Yes Yes    
29881 08/19/13   Werner/ Ramona No Yes Yes Yes    
29882 08/19/13   Werner/ Ramona Yes No Yes Yes    
29883     Werner/ Ramona Yes Yes Yes Yes    
29884     Werner/ Ramona Yes Yes Yes Yes    
29885     Werner/ Ramona Yes Yes Yes Yes    
>
>
29879 08/19/13

29879_0.5_0.data

29879_0.5_1.data

29879_0.5_2.data

29879_0.5_3.data

 Ramona Yes Yes Yes Yes    
29880 08/19/13

29880_0.5_0.data

29880_0.5_0.data

29880_0.5_0.data

 Ramona Yes No Yes Yes    
29881 08/19/13

29881_0.5_1.data

29881_0.5_2.data

29881_0.5_3.data

 Ramona No Yes Yes Yes    
29882 08/19/13

29882_0.5_0.data

29882_0.5_2.data

29882_0.5_3.data

 Ramona Yes No Yes Yes    
29883 08/19/13   Werner/Ramona Yes Yes Yes Yes    
29884 08/19/13

29884_0.5_0.data

29884_0.5_1.data

29884_0.5_2.data

29884_0.5_3.data

 Ramona Yes Yes Yes Yes    
29885 08/19/13

29885_0.5_0.data

29885_0.5_1.data

29885_0.5_2.data

29885_0.5_3.data

 Ramona Yes Yes Yes Yes    
 
29890                  
29891                  
29892                  
Line: 126 to 126
 
29902 08/20/13   Douglas No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.  
29904 08/20/13   Pierre/ Ramona No No No No    
29905 08/20/13   Pierre/ Ramona No No No No    
Changed:
<
<
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Omar/ Ramona

Douglas

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise

  
29907 08/20/13

29907_0.5_0.data

29907_0.5_1.data

29907_0.5_2.data

29907_0.5_3.data

 Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)  
29908 08/20/13

29908_0.5_0.data

29908_0.5_2.data

29908_0.5_3.data

Pierre

Douglas

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.

  
29909 08/20/13

29909_0.5_0.data

29909_0.5_1.data

29909_0.5_2.data

29909_0.5_3.data

 Ramona/ Pierre Yes Yes Yes Yes    
29910 08/20/13

29910_0.5_1.data

29910_0.5_2.data

29910_0.5_3.data

 Ramona/ Pierre No Yes Yes Yes    
>
>
29906 08/20/13 29906_0.5_0_PA.data

29906_0.5_1_PA.data

29906_0.5_2_PA.data

29906_0.5_3_PA.data

29906_0.5_0_PA.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Pierre (PA)

Douglas (notes)

Ramona

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise

  
29907 08/20/13

29907_0.5_0_PA.data

29907_0.5_1_PA.data

29907_0.5_2_PA.data

29907_0.5_3_PA.data

29907_0.5_0.data

29907_0.5_1.data

29907_0.5_2.data

29907_0.5_3.data

Pierre (notes, PA)

Ramona

 Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)  
29908 08/20/13

29908_0.5_0_PA.data

29908_0.5_2_PA.data

29908_0.5_3_PA.data

29908_0.5_2.data

29908_0.5_3.data

Pierre (PA)

Douglas (notes)

Ramona

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.

  
29909 08/20/13

29909_0.5_0_PA.data

29909_0.5_1_PA.data

29909_0.5_2_PA.data

29909_0.5_3_PA.data

29909_0.5_0.data

29909_0.5_1.data

29909_0.5_2.data

29909_0.5_3.data

Pierre (PA)

Ramona

 Yes Yes Yes Yes    
29910 08/20/13

29910_0.5_1_PA.data

29910_0.5_2_PA.data

29910_0.5_3_PA.data

29910_0.5_1.data

29910_0.5_2.data

29910_0.5_3.data

Pierre (PA)

Ramona

 No Yes Yes Yes    
 
29911 08/20/13   Douglas No No No No    
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

 Douglas No Yes Yes Yes    
29914 08/20/13

29914_0.5_1.data

29914_0.5_2.data

29914_0.5_3.data

 Douglas No Yes Yes Yes    
Line: 143 to 143
 
29921 08/20/13

29921_0.5_2.data

29921_0.5_3.data

 Douglas No No Yes Yes    
29922 08/20/13

29922_0.5_1.data

29922_0.5_2.data

29922_0.5_3.data

 Douglas No Yes Yes Yes    
29923 08/20/13

29923_0.5_1.data

29923_0.5_2.data

29923_0.5_3.data

 Douglas No Yes Yes Yes    
Changed:
<
<
29924 08/20/13

29924_0.5_0.data

29924_0.5_1.data

29924_0.5_2.data

29924_0.5_3.data

Ramona/ Omar

Douglas

 No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.  
29925 08/20/13

29925_0.5_1.data

29925_0.5_2.data

29925_0.5_3.data

 Douglas No Yes Yes Yes    
>
>
29924 08/20/13

29924_0.5_1_DT.data

29924_0.5_2_DT.data

29924_0.5_3_DT.data

29924_0.5_1.data

29924_0.5_2.data

29924_0.5_3.data

Omar (notes)

Douglas (DT)

Ramona

 No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.  
29925 08/20/13

29925_0.5_1.data

29925_0.5_2.data

29925_0.5_3.data

Douglas

 No Yes Yes Yes    
 
29926 08/20/13   Douglas No No No No    
29927 08/20/13   Douglas No No No No    
29928 08/20/13   Ramona No Yes Yes Yes    
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.  
29930 08/20/13   Douglas No No No No All channels mostly noise.  
Changed:
<
<
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes    
>
>
29931 08/20/13

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes    
 
29932                  
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera/Omar No No No No Every channel was only noise  
29934                  
Line: 176 to 176
 
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts  
29956                  
29957                  
Changed:
<
<
29958 08/21/13   Ramona No Yes Yes Yes    
>
>
29958 08/21/13

29958_0.5_1.data

29958_0.5_2.data

29958_0.5_3.data

 Ramona No Yes Yes Yes    
 
29959                  
Changed:
<
<
29960 08/21/13   Ramona No Yes Yes Yes    
>
>
29960 08/21/13

29960_0.5_1.data

29960_0.5_2.data

29960_0.5_3.data

 Ramona No Yes Yes Yes    
 
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s  
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise  
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise  
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s

  
Changed:
<
<
29966 08/22/13   Ramona No Yes Yes Yes    
>
>
29966 08/22/13

29966_0.5_1.data

29966_0.5_3.data

29966_0.5_3.data

 Ramona No Yes Yes Yes    
 
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise

  
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s

  
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

29971_0.5_2.data

29971_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful between t = .100s to t = .310s  
Changed:
<
<
29972 08/22/13   Ramona No Yes Yes Yes    
>
>
29972 08/22/13

29972_0.5_1.data

29972_0.5_2.data

29972_0.5_3.data

 Ramona No Yes Yes Yes    
 
29974 08/22/13

29974_0.5_0.data

29974_0.5_1.data

29974_0.5_2.data

29974_0.5_3.data

 Javiera No No No No Every channel was only noise  
Changed:
<
<
29975 08/22/13

29975_0.5_0.data

29975_0.5_1.data

29975_0.5_2.data

29975_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch2, Ch3: Most useful between t = .1s to t = .3s  
29976 08/22/13

29976_0.5_0.data

29976_0.5_1.data

29976_0.5_2.data

29976_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Most useful between t = .1s to t = .27s  
>
>
29975 08/22/13

29975_0.5_1.data

29975_0.5_2.data

29975_0.5_3.data

Javiera (notes)

Ramona

No

 Yes Yes Yes Ch2, Ch3: Most useful between t = .1s to t = .3s  
29976 08/22/13

29976_0.5_1.data

29976_0.5_2.data

29976_0.5_3.data

Javiera (notes)

Ramona

 No Yes Yes Yes Ch1, Ch2, Ch3: Most useful between t = .1s to t = .27s  
 
29978 08/22/13

29978_0.5_0.data

29978_0.5_1.data

29978_0.5_2.data

29978_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .3s, everything afterwards is just noise  
Changed:
<
<
29980 08/22/13

29980_0.5_0.data

29980_0.5_1.data

29980_0.5_2.data

29980_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .3s, everything afterwards is just noise  
>
>
29980 08/22/13

29980_0.5_1.data

29980_0.5_2.data

29980_0.5_3.data

Javiera (notes)

Ramona

 No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .3s, everything afterwards is just noise  
 
29981 08/22/13

29981_0.5_0.data

29981_0.5_1.data

29981_0.5_2.data

29981_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .33s, everything afterwards is just noise  
29982 08/22/13

29982_0.5_0.data

29982_0.5_1.data

29982_0.5_2.data

29982_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .35s. Each one had a last voltage peak at around t = .351s with a v = 3.4  
29983 08/22/13

29983_0.5_0.data

29983_0.5_1.data

29983_0.5_2.data

29983_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: All of these are useful between t = .05s to t = .35s. In each one there is a large voltage peak at around t - .35s with a voltage of about 3.4V  

Revision 1182014-08-27 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 60 to 60
  Yes
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes  
Changed:
<
<
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

   No Yes        
>
>
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes        
 
29807                  
29808                  
29809                  

Revision 1172014-08-04 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 333 to 333
 
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy signal with large noise peaks at 0.123 s (~1.0 V), 0.342 s (~0.85 V), & 0.364 s (~1.50 V) with inconsistent peak shapes but enough peaks to collect.

Ch 1 is a good signal with a large signal peak at 0.363 s (~3.30 V).

Ch 2 is a good signal with an over saturated signal at 0.366 s.

Ch 3 is a good signal with a large peak signal at 0.364 s (~1.80 V).

  
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre No No No No No signals but noise.  
30160 09/11/13

30160_0.5_0.data

30160_0.5_1.data

30160_0.5_2.data

30160_0.5_3.data

 Pierre No No No No No signals but noise. Ch 2 & Ch 3 has large periodic noise signals.  
Changed:
<
<
30162 09/11/13

30162_0.5_0.data

30162_0.5_1.data

30162_0.5_2.data

30162_0.5_3.data

 Pierre            
>
>
30162 09/11/13

30162_0.5_0.data

30162_0.5_1.data

30162_0.5_2.data

30162_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has inconsistent peak shapes but is low in noise.

Ch 1 has a good signal with an oversaturated signal at 0.300 s.

Ch 2 has a good signal with an oversaturated signal at 0.300 s.

Ch 3 has a good signal with an oversaturated signal at 0.300 s.

  
 
30163 09/11/13                
30164 09/11/13                
30165 09/11/13                

Revision 1162014-08-04 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 331 to 331
 
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual, some reflected peaks and has no peaks beyond 0.3 V.

Ch 1 is mostly clean and peak shapes are good except towards the end of the shot.

Ch 2 has a noisy baseline but is otherwise clean and good peak shapes.

Ch 3 has some large peaks but is otherwise clean and has consistent peak shapes.

  
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual and there are discernible peaks but may not be very good for generating rates.

Ch 1 has a good signal with one large peak at 0.329 (~ 3.0 V)

Ch 2 has a good signal with a large peak at 0.328 (~ 2.3 V)

Ch 3 has a good signal with a large reflected peak at 0.327 (~ 1.4 V)

  
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy signal with large noise peaks at 0.123 s (~1.0 V), 0.342 s (~0.85 V), & 0.364 s (~1.50 V) with inconsistent peak shapes but enough peaks to collect.

Ch 1 is a good signal with a large signal peak at 0.363 s (~3.30 V).

Ch 2 is a good signal with an over saturated signal at 0.366 s.

Ch 3 is a good signal with a large peak signal at 0.364 s (~1.80 V).

  
Changed:
<
<
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre            
30160 09/11/13

30160_0.5_0.data

30160_0.5_1.data

30160_0.5_2.data

30160_0.5_3.data

 Pierre            
>
>
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre No No No No No signals but noise.  
30160 09/11/13

30160_0.5_0.data

30160_0.5_1.data

30160_0.5_2.data

30160_0.5_3.data

 Pierre No No No No No signals but noise. Ch 2 & Ch 3 has large periodic noise signals.  
 
30162 09/11/13

30162_0.5_0.data

30162_0.5_1.data

30162_0.5_2.data

30162_0.5_3.data

 Pierre            
Changed:
<
<
30163                  
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30169                  
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30172                  
30173                  
30174                  
30175                  
30176                  
30177                  
30178                  
30179                  
>
>
30163 09/11/13                
30164 09/11/13                
30165 09/11/13                
30166 09/11/13                
30167 09/11/13                
30168 09/11/13                
30169 09/11/13                
30170 09/11/13                
30171 09/11/13                
30172 09/11/13                
30173 09/11/13                
30174 09/11/13                
30175 09/11/13                
30176 09/11/13                
30177 09/11/13                
30178 09/11/13                
30179 09/11/13                
 
30180 09/12/13

30180_0.5_0.data

30180_0.5_1.data

30180_0.5_2.data

30180_0.5_3.data

 Omar No No No No All four channels were composed of noise.  
30181 09/12/13

30181_0.5_0.data

30181_0.5_1.data

30181_0.5_2.data

30181_0.5_3.data

 Omar No No No No All channels are composed of noise.  
30182 09/12/13

30182_0.5_0.data

30182_0.5_1.data

30182_0.5_2.data

30182_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks. Channel 1 has a sharp decrease in data at ~.35s.  
Line: 358 to 358
 
30184 09/12/13

30184_0.5_0.data

30184_0.5_1.data

30184_0.5_2.data

30184_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30185 09/12/13

30185_0.5_0.data

30185_0.5_1.data

30185_0.5_2.data

30185_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30187 09/12/13

30187_0.5_0.data

30187_0.5_1.data

30187_0.5_2.data

30187_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks. All other channels have a sharp decrease in data at ~.29s.  
Changed:
<
<
30188                  
30189                  
30190                  
>
>
30188 09/12/13

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30188_0.5_1.data

30188_0.5_2.data

30188_0.5_3.data

              
30189 09/12/13

30189_0.5_0.data

30189_0.5_1.data

30189_0.5_2.data

30189_0.5_3.data

              
30190 09/12/13

30190_0.5_0.data

30190_0.5_1.data

30190_0.5_2.data

30190_0.5_3.data

              
 
30191                  
30192                  
30193                  

Revision 1152014-07-31 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 330 to 330
 
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak at 0.122 s (~1.0 V) and at 0.250 s (~0.80 V). Ch 0 as usual is noisy with bad peak shapes but still distinguishable.

Ch 1 has over-saturated signals between 0.165 s to 0.200 s and at 0.253 s but has clean, consistent peak shapes.

Ch 2 has over-saturated signals at 0.192 s and at 0.249 s but has clean, consistent peaks.

Ch 3 has low rates at 0.193 s but has clean, consistent peak shapes.

  
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual, some reflected peaks and has no peaks beyond 0.3 V.

Ch 1 is mostly clean and peak shapes are good except towards the end of the shot.

Ch 2 has a noisy baseline but is otherwise clean and good peak shapes.

Ch 3 has some large peaks but is otherwise clean and has consistent peak shapes.

  
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual and there are discernible peaks but may not be very good for generating rates.

Ch 1 has a good signal with one large peak at 0.329 (~ 3.0 V)

Ch 2 has a good signal with a large peak at 0.328 (~ 2.3 V)

Ch 3 has a good signal with a large reflected peak at 0.327 (~ 1.4 V)

  
Changed:
<
<
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre            
>
>
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy signal with large noise peaks at 0.123 s (~1.0 V), 0.342 s (~0.85 V), & 0.364 s (~1.50 V) with inconsistent peak shapes but enough peaks to collect.

Ch 1 is a good signal with a large signal peak at 0.363 s (~3.30 V).

Ch 2 is a good signal with an over saturated signal at 0.366 s.

Ch 3 is a good signal with a large peak signal at 0.364 s (~1.80 V).

  
 
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre            
30160 09/11/13

30160_0.5_0.data

30160_0.5_1.data

30160_0.5_2.data

30160_0.5_3.data

 Pierre            
30162 09/11/13

30162_0.5_0.data

30162_0.5_1.data

30162_0.5_2.data

30162_0.5_3.data

 Pierre            

Revision 1142014-07-28 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 329 to 329
 
30154 09/10/13

30154_0.5_0.data

30154_0.5_1.data

30154_0.5_2.data

30154_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with large noise peaks (2.0 V & 1.2 V) at 0.333 s and at 0.402 V.

Ch 1 has an over-saturated signal at 0.197 s, 0.237 s, 0.336 s, & 0.403s. Ch 1 is a bit noisy making some peak shapes noisy.

Ch 2 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

Ch 3 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

  
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak at 0.122 s (~1.0 V) and at 0.250 s (~0.80 V). Ch 0 as usual is noisy with bad peak shapes but still distinguishable.

Ch 1 has over-saturated signals between 0.165 s to 0.200 s and at 0.253 s but has clean, consistent peak shapes.

Ch 2 has over-saturated signals at 0.192 s and at 0.249 s but has clean, consistent peaks.

Ch 3 has low rates at 0.193 s but has clean, consistent peak shapes.

  
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual, some reflected peaks and has no peaks beyond 0.3 V.

Ch 1 is mostly clean and peak shapes are good except towards the end of the shot.

Ch 2 has a noisy baseline but is otherwise clean and good peak shapes.

Ch 3 has some large peaks but is otherwise clean and has consistent peak shapes.

  
Changed:
<
<
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre            
>
>
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual and there are discernible peaks but may not be very good for generating rates.

Ch 1 has a good signal with one large peak at 0.329 (~ 3.0 V)

Ch 2 has a good signal with a large peak at 0.328 (~ 2.3 V)

Ch 3 has a good signal with a large reflected peak at 0.327 (~ 1.4 V)

  
 
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre            
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre            
30160 09/11/13

30160_0.5_0.data

30160_0.5_1.data

30160_0.5_2.data

30160_0.5_3.data

 Pierre            

Revision 1132014-07-24 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 328 to 328
 
30153 09/10/13

30153_0.5_0.data

30153_0.5_1.data

30153_0.5_2.data

30153_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with inconsistent peak shapes.

Ch 1 has an over-saturated signal at 0.252 s with some reflected peaks throughout the shot.

Ch 2 has an oversaturated signal at 0.25 s but is otherwise clean.

Ch 3 has an over-saturated signal at 0.25 s but is otherwise clean.

  
30154 09/10/13

30154_0.5_0.data

30154_0.5_1.data

30154_0.5_2.data

30154_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with large noise peaks (2.0 V & 1.2 V) at 0.333 s and at 0.402 V.

Ch 1 has an over-saturated signal at 0.197 s, 0.237 s, 0.336 s, & 0.403s. Ch 1 is a bit noisy making some peak shapes noisy.

Ch 2 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

Ch 3 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

  
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak at 0.122 s (~1.0 V) and at 0.250 s (~0.80 V). Ch 0 as usual is noisy with bad peak shapes but still distinguishable.

Ch 1 has over-saturated signals between 0.165 s to 0.200 s and at 0.253 s but has clean, consistent peak shapes.

Ch 2 has over-saturated signals at 0.192 s and at 0.249 s but has clean, consistent peaks.

Ch 3 has low rates at 0.193 s but has clean, consistent peak shapes.

  
Changed:
<
<
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre            
>
>
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is noisy as usual, some reflected peaks and has no peaks beyond 0.3 V.

Ch 1 is mostly clean and peak shapes are good except towards the end of the shot.

Ch 2 has a noisy baseline but is otherwise clean and good peak shapes.

Ch 3 has some large peaks but is otherwise clean and has consistent peak shapes.

  
 
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre            
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre            
30159 09/11/13

30159_0.5_0.data

30159_0.5_1.data

30159_0.5_2.data

30159_0.5_3.data

 Pierre            

Revision 1122014-07-23 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 327 to 327
 
30152 09/10/13

30152_0.5_0.data

30152_0.5_1.data

30152_0.5_2.data

30152_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a very noisy baseline and noisy peaks, the signal ends at 0.245 s.

Ch 1 has a clean signal and ends at 0.25 s with an over-saturated signal.

Ch 2 has a clean signal and also ends at 0.25 s with an over-saturated signal.

Ch 3 has a clean signal and also ends at 0.25 s with an over-saturated signal.

  
30153 09/10/13

30153_0.5_0.data

30153_0.5_1.data

30153_0.5_2.data

30153_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with inconsistent peak shapes.

Ch 1 has an over-saturated signal at 0.252 s with some reflected peaks throughout the shot.

Ch 2 has an oversaturated signal at 0.25 s but is otherwise clean.

Ch 3 has an over-saturated signal at 0.25 s but is otherwise clean.

  
30154 09/10/13

30154_0.5_0.data

30154_0.5_1.data

30154_0.5_2.data

30154_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with large noise peaks (2.0 V & 1.2 V) at 0.333 s and at 0.402 V.

Ch 1 has an over-saturated signal at 0.197 s, 0.237 s, 0.336 s, & 0.403s. Ch 1 is a bit noisy making some peak shapes noisy.

Ch 2 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

Ch 3 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

  
Changed:
<
<
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

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 Pierre            
>
>
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak at 0.122 s (~1.0 V) and at 0.250 s (~0.80 V). Ch 0 as usual is noisy with bad peak shapes but still distinguishable.

Ch 1 has over-saturated signals between 0.165 s to 0.200 s and at 0.253 s but has clean, consistent peak shapes.

Ch 2 has over-saturated signals at 0.192 s and at 0.249 s but has clean, consistent peaks.

Ch 3 has low rates at 0.193 s but has clean, consistent peak shapes.

  
 
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre            
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre            
30158 09/10/13

30158_0.5_0.data

30158_0.5_1.data

30158_0.5_2.data

30158_0.5_3.data

 Pierre            

Revision 1112014-07-23 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 326 to 326
 
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~3.30 V) at 0.328 s otherwise is the cleanest ch 0 signal I have seen.

Ch 1 has several gaps of over-saturation from 0.243 s to 0.317 s. Peaks are a little noisy but still consistent.

Ch 2 has a large peak (~2.55 V) at 0.315 s but is otherwise clean with consistent peaks.

Ch 3 has a large peak (~3.30 V) at 0.330 s but is otherwise clean with consistent peaks.

  
30152 09/10/13

30152_0.5_0.data

30152_0.5_1.data

30152_0.5_2.data

30152_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a very noisy baseline and noisy peaks, the signal ends at 0.245 s.

Ch 1 has a clean signal and ends at 0.25 s with an over-saturated signal.

Ch 2 has a clean signal and also ends at 0.25 s with an over-saturated signal.

Ch 3 has a clean signal and also ends at 0.25 s with an over-saturated signal.

  
30153 09/10/13

30153_0.5_0.data

30153_0.5_1.data

30153_0.5_2.data

30153_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with inconsistent peak shapes.

Ch 1 has an over-saturated signal at 0.252 s with some reflected peaks throughout the shot.

Ch 2 has an oversaturated signal at 0.25 s but is otherwise clean.

Ch 3 has an over-saturated signal at 0.25 s but is otherwise clean.

 
Changed:
<
<
30154 09/10/13

30154_0.5_0.data

30154_0.5_1.data

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 Pierre            
>
>
30154 09/10/13

30154_0.5_0.data

30154_0.5_1.data

30154_0.5_2.data

30154_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with large noise peaks (2.0 V & 1.2 V) at 0.333 s and at 0.402 V.

Ch 1 has an over-saturated signal at 0.197 s, 0.237 s, 0.336 s, & 0.403s. Ch 1 is a bit noisy making some peak shapes noisy.

Ch 2 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

Ch 3 has an over-saturated signal at 0.333 s, & 0.400 s but is otherwise clean with consistent peaks.

  
 
30155 09/10/13

30155_0.5_0.data

30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre            
30156 09/10/13

30156_0.5_0.data

30156_0.5_1.data

30156_0.5_2.data

30156_0.5_3.data

 Pierre            
30157 09/10/13

30157_0.5_0.data

30157_0.5_1.data

30157_0.5_2.data

30157_0.5_3.data

 Pierre            

Revision 1102014-07-21 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 324 to 324
 
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

  
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

Ch 3 has periods of low rates at 0.264 s, 0.336 s, 0.392 s with a few short periods of over-saturation. There are also many reflected peaks namely from 0.414 s until the end.

  
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~3.30 V) at 0.328 s otherwise is the cleanest ch 0 signal I have seen.

Ch 1 has several gaps of over-saturation from 0.243 s to 0.317 s. Peaks are a little noisy but still consistent.

Ch 2 has a large peak (~2.55 V) at 0.315 s but is otherwise clean with consistent peaks.

Ch 3 has a large peak (~3.30 V) at 0.330 s but is otherwise clean with consistent peaks.

  
Changed:
<
<
30152 09/10/13

30152_0.5_0.data

30152_0.5_1.data

30152_0.5_2.data

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 Pierre            
30153 09/10/13

30153_0.5_0.data

30153_0.5_1.data

30153_0.5_2.data

30153_0.5_3.data

 Pierre            
>
>
30152 09/10/13

30152_0.5_0.data

30152_0.5_1.data

30152_0.5_2.data

30152_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a very noisy baseline and noisy peaks, the signal ends at 0.245 s.

Ch 1 has a clean signal and ends at 0.25 s with an over-saturated signal.

Ch 2 has a clean signal and also ends at 0.25 s with an over-saturated signal.

Ch 3 has a clean signal and also ends at 0.25 s with an over-saturated signal.

  
30153 09/10/13

30153_0.5_0.data

30153_0.5_1.data

30153_0.5_2.data

30153_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a noisy signal with inconsistent peak shapes.

Ch 1 has an over-saturated signal at 0.252 s with some reflected peaks throughout the shot.

Ch 2 has an oversaturated signal at 0.25 s but is otherwise clean.

Ch 3 has an over-saturated signal at 0.25 s but is otherwise clean.

 
 
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30154_0.5_1.data

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 Pierre            
30155 09/10/13

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30155_0.5_1.data

30155_0.5_2.data

30155_0.5_3.data

 Pierre            
30156 09/10/13

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30156_0.5_2.data

30156_0.5_3.data

 Pierre            

Revision 1092014-07-21 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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Line: 324 to 324
 
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

  
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

Ch 3 has periods of low rates at 0.264 s, 0.336 s, 0.392 s with a few short periods of over-saturation. There are also many reflected peaks namely from 0.414 s until the end.

  
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~3.30 V) at 0.328 s otherwise is the cleanest ch 0 signal I have seen.

Ch 1 has several gaps of over-saturation from 0.243 s to 0.317 s. Peaks are a little noisy but still consistent.

Ch 2 has a large peak (~2.55 V) at 0.315 s but is otherwise clean with consistent peaks.

Ch 3 has a large peak (~3.30 V) at 0.330 s but is otherwise clean with consistent peaks.

  
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30154 09/10/13

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30155 09/10/13

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30156 09/10/13

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30157 09/10/13

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30158 09/10/13

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 Pierre            
30159 09/11/13

30159_0.5_0.data

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 Pierre            
30160 09/11/13

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30160_0.5_1.data

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30160_0.5_3.data

 Pierre            
30162 09/11/13

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30162_0.5_1.data

30162_0.5_2.data

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 Pierre            
 
30163                  
30164                  
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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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Line: 323 to 323
 
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

  
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

Ch 3 has periods of low rates at 0.264 s, 0.336 s, 0.392 s with a few short periods of over-saturation. There are also many reflected peaks namely from 0.414 s until the end.

  
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30151 09/10/13

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>
>
30151 09/10/13

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30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~3.30 V) at 0.328 s otherwise is the cleanest ch 0 signal I have seen.

Ch 1 has several gaps of over-saturation from 0.243 s to 0.317 s. Peaks are a little noisy but still consistent.

Ch 2 has a large peak (~2.55 V) at 0.315 s but is otherwise clean with consistent peaks.

Ch 3 has a large peak (~3.30 V) at 0.330 s but is otherwise clean with consistent peaks.

  
 
30152                  
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Revision 1072014-07-16 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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Line: 322 to 322
 
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

  
Changed:
<
<
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes    

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

  
>
>
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

Ch 3 has periods of low rates at 0.264 s, 0.336 s, 0.392 s with a few short periods of over-saturation. There are also many reflected peaks namely from 0.414 s until the end.

  
 
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

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30152                  
30153                  

Revision 1062014-07-16 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 322 to 322
 
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

  
Changed:
<
<
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

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 Pierre No Yes    

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

  
>
>
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes    

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

Ch 2 has periods of over-saturation at 0.266 s, 0.337 s, 0.390 s, and at 0.440 s there is a large noise peak (~ 1.60 V). The peaks are a little noisy but still consistent enough to use.

  
 
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

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 Pierre            
30152                  
30153                  

Revision 1052014-07-16 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 322 to 322
 
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

 
Changed:
<
<
30150 09/10/13

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>
>
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre No Yes    

Ch 0 has so many noise peaks greater than 0.6 V (mostly around ~1.5 V) where the particle peaks are no more than 0.3 V and have inconsistent shapes.

Ch 1 has periods of over-saturation during 0.173-0.275 s, 0.340 s, 0.393 s, 0.444-0.471 s that are reminiscent of sawtooth and/or fishbones.

  
 
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre            
30152                  
30153                  

Revision 1042014-07-15 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 321 to 321
 
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
Changed:
<
<
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre            
>
>
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a noisy channel with large noise peaks and the peaks are inconsistent in shape. May not produce good rates.

Ch 1 has a gap of over-saturation from 0.168 to 0.230 with occasional large peaks (~ 1.66 V)

Ch 2 has large peaks at 0.201 (~ 2.33 V), 0.205 (~ 2.00), 0.432 (~ 2.50) and a gap of over-saturation from 0.168 to 0.218.

Ch 3 has smaller gaps of over-saturation with sections of peaks mixed in between the times 0.160 to 0.280. Also, large peaks at 0.167 (~ 1.8 V), and 0.214 (~ 1.80 V).

 
 
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre            
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre            
30152                  

Revision 1032014-07-14 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 320 to 320
 
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
Changed:
<
<
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec and periods of over-saturation of signal but peaks are clean and consistent.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections but peaks are clean and consistent.

  
>
>
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal. Peaks are not as clean and consistent as Ch 1 but not worse than Ch 0.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections. Peaks are clean and consistent as Ch 1 but not worse than Ch 0.

  
 
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre            
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre            
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre            

Revision 1022014-07-14 - clope023

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 258 to 258
 
30079 09/06/2013

30079_0.5_0.data

30079_0.5_1.data

30079_0.5_2.data

30079_0.5_3.data

 Carlos Lopez No No No No No channel contains data  
30080 09/06/2013

30080_0.5_0.data

30080_0.5_1.data

30080_0.5_2.data

30080_0.5_3.data

 Carlos Lopez No No No No No channel contains data  
30081 09/06/2013

30081_0.5_0.data

30081_0.5_1.data

30081_0.5_2.data

30081_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: no data  
Changed:
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<
30082                  
30084                  
30085                  
30086                  
>
>
30082 09/06/2013

30082_0.5_0.data

30082_0.5_1.data

30082_0.5_2.data

30082_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
30084 09/06/2013

30084_0.5_0.data

30084_0.5_1.data

30084_0.5_2.data

30084_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
30085 09/06/2013

30085_0.5_0.data

30085_0.5_1.data

30085_0.5_2.data

30085_0.5_3.data

 Carlos Lopez No No No No None of the channels have data  
30086 09/06/2013

30086_0.5_0.data

30086_0.5_1.data

30086_0.5_2.data

30086_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: no usable data  
 
30087                  
30088                  
30089                  

Revision 1012014-07-14 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 320 to 320
 
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
Changed:
<
<
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre            
>
>
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has noisy peaks (~ 3.33 V) during 0.123-0.235 sec as well as noisy peaks that are somewhat consistent.

Ch 1 has large noise peaks (~ 3.33 V) during 0.123-0.235 sec with periods of over-saturation of signal but peaks are clean and consistent.

Ch 2 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec and periods of over-saturation of signal but peaks are clean and consistent.

Ch 3 has the same large noise peaks (~ 3.33 V) during 0.123-0.235 sec but no over-saturation sections but peaks are clean and consistent.

  
 
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre            
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre            
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre            

Revision 1002014-07-14 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 319 to 319
 
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 peaks are riddled with noise making it extremely difficult to fond consistent peaks.

Ch 1 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 2 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 3 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

  
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
Changed:
<
<
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre            
>
>
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few large noise peaks between 0.342-0.490 sec and besides the latter no peaks exceed 0.3 V.

Ch 1 has a large noise peak (~ -2.20 V) at 0.467 sec but is otherwise a good signal.

Ch 2 has a large noise peak (~ -1.30 V) at 0.467 sec but is otherwise a good signal.

Ch 3 has a noisy baseline but peaks are clean and consistent.

  
 
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre            
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre            
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre            

Revision 992014-07-14 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 319 to 319
 
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 peaks are riddled with noise making it extremely difficult to fond consistent peaks.

Ch 1 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 2 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 3 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

  
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
Changed:
<
<
30147                  
30148                  
30149                  
30150                  
30151                  
>
>
30147 09/10/13

30147_0.5_0.data

30147_0.5_1.data

30147_0.5_2.data

30147_0.5_3.data

 Pierre            
30148 09/10/13

30148_0.5_0.data

30148_0.5_1.data

30148_0.5_2.data

30148_0.5_3.data

 Pierre            
30149 09/10/13

30149_0.5_0.data

30149_0.5_1.data

30149_0.5_2.data

30149_0.5_3.data

 Pierre            
30150 09/10/13

30150_0.5_0.data

30150_0.5_1.data

30150_0.5_2.data

30150_0.5_3.data

 Pierre            
30151 09/10/13

30151_0.5_0.data

30151_0.5_1.data

30151_0.5_2.data

30151_0.5_3.data

 Pierre            
 
30152                  
30153                  
30154                  

Revision 982014-07-14 - clope023

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 254 to 254
 
30075 09/05/2013

30075_0.5_0.data

30075_0.5_1.data

30075_0.5_2.data

30075_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30076 09/05/2013

30076_0.5_0.data

30076_0.5_1.data

30076_0.5_2.data

30076_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30077 09/05/2013

30077_0.5_0.data

30077_0.5_1.data

30077_0.5_2.data

30077_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
Changed:
<
<
30078                  
30079                  
30080                  
30081                  
>
>
30078 09/06/2013

30078_0.5_0.data

30078_0.5_1.data

30078_0.5_2.data

30078_0.5_3.data

 Carlos Lopez No No No No No channel contains data  
30079 09/06/2013

30079_0.5_0.data

30079_0.5_1.data

30079_0.5_2.data

30079_0.5_3.data

 Carlos Lopez No No No No No channel contains data  
30080 09/06/2013

30080_0.5_0.data

30080_0.5_1.data

30080_0.5_2.data

30080_0.5_3.data

 Carlos Lopez No No No No No channel contains data  
30081 09/06/2013

30081_0.5_0.data

30081_0.5_1.data

30081_0.5_2.data

30081_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: no data  
 
30082                  
30084                  
30085                  

Revision 972014-07-12 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 318 to 318
 
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is riddled with so much noise that most peaks are impossible to distinguish from noise.

Ch 1 has a large reflected peak (~ -3.31 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 2 has a large reflected peak (~ -3.04 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 3 has a large reflected peak (~ -2.67 V) at 0.440 sec but otherwise has clean consistent peaks.

  
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 peaks are riddled with noise making it extremely difficult to fond consistent peaks.

Ch 1 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 2 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 3 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

  
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
Changed:
<
<
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

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 Pierre            
>
>
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few noise peaks but has peaks that are somewhat consistent but this signal still has a lot of noise.

Ch 1 has a good signal with consistent peaks save for a oversaturated signal at 0.402 sec.

Ch 2 has a noiser baseline signal with the same oversaturated signal at 0.402 sec.

Ch 3 has a clean signal with little noise.

  
 
30147                  
30148                  
30149                  

Revision 962014-07-11 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 317 to 317
 
30141 09/10/13

30141_0.5_0.data

30141_0.5_1.data

30141_0.5_2.data

30141_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.26 V with very noisy peaks.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has some noise but otherwise clean, consistent peaks.

Ch 3 has a clean signal with good peaks.

  
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is riddled with so much noise that most peaks are impossible to distinguish from noise.

Ch 1 has a large reflected peak (~ -3.31 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 2 has a large reflected peak (~ -3.04 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 3 has a large reflected peak (~ -2.67 V) at 0.440 sec but otherwise has clean consistent peaks.

  
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 peaks are riddled with noise making it extremely difficult to fond consistent peaks.

Ch 1 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 2 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 3 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

  
Changed:
<
<
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes    

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

  
>
>
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

Ch 2 has large reflected peaks (~ -1.20) at 0.419 and 0.441 and another (~ -1.60) at 0.473 sec otherwise channel is has some noise but peaks are consistent.

ch 3 has large reflected peaks (~ -1.0) at 0.420 and 0.442 and another (~ -1.20) at 0.472 sec otherwise channel is has some noise but peaks are consistent.

  
 
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre            
30147                  
30148                  

Revision 952014-07-11 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 316 to 316
 
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.27 V and has a lot of noise that peaks inconsistent in shape.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has a clean signal with some noise in the baseline.

Ch 3 has a clean signal with some noise in the baseline.

  
30141 09/10/13

30141_0.5_0.data

30141_0.5_1.data

30141_0.5_2.data

30141_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.26 V with very noisy peaks.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has some noise but otherwise clean, consistent peaks.

Ch 3 has a clean signal with good peaks.

  
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is riddled with so much noise that most peaks are impossible to distinguish from noise.

Ch 1 has a large reflected peak (~ -3.31 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 2 has a large reflected peak (~ -3.04 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 3 has a large reflected peak (~ -2.67 V) at 0.440 sec but otherwise has clean consistent peaks.

  
Changed:
<
<
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre            
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre            
>
>
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 peaks are riddled with noise making it extremely difficult to fond consistent peaks.

Ch 1 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 2 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

Ch 3 has a large reflected peak (~ -1.0 V) at 0.430 sec but is otherwise a good signal with consistent peak shapes.

  
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre Yes Yes    

Ch 0 has large peaks (~ 0.8 V) at 0.418 and 0.442 sec with a few more trailing at the end of the shot. Peaks are somewhat consistent.

Ch 1 has large reflected peaks (~ -2.0 V) at 0.441 and 0.472 sec but it otherwise a good signal with clean, consistent peaks.

  
 
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre            
30147                  
30148                  

Revision 942014-07-10 - jlatorre1513

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Revision 932014-07-10 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 311 to 311
 
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
30136 09/10/13

30136_0.5_0.data

30136_0.5_1.data

30136_0.5_2.data

30136_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large peaks at 0.209 and 0.300 sec (~1.0 V) and a noise peak (~1.0 V) at 0.500 sec. The peaks in this channel are drowned with noise and are inconsistent in shape.

Ch 1 has a few sections of over saturated signals from 0.190 to 0.309 sec.

Ch 2 has a noisy baseline but the peaks are consistent in shape.

Ch 3 has a clean signal.

  
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

Ch 2 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. The baseline signal is somewhat noisy but a mojority of paritcle peaks have clean shapes.

Ch 3 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. This channel also has gaps of no activity but other than that is clean and had good peaks.

  
Changed:
<
<
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~0.68 V) at 0.069 sec and has no other peaks larger than 0.26 V. This channel also has high frequency signals that are disgused within particle peaks. Zoom in to differentiate.

Ch 1 is a clean signal with consistent peak shapes.

Ch 2 is decently clean with good peaks but some noise embedded in the baseline signal.

Ch 3 is a clean signal

  
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a grouping of high frequency noise (~0.60 V) at 0.387 sec alongside not having any particle peaks above 0.25 V.

Ch 1 is a clean signal with good peak shapes.

Ch 2 is a clean signal with some noise in the baseline but the peaks are consistent.

Ch 3 has a large peak (~2.70 V) at 0.246 sec and prevelant noise in the baseline but otherwise clean good peaks.

  
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.27 V and has a lot of noise that peaks inconsistent in shape.

Ch 1 is a clean signal with consistent peak shapes.

Ch 2 is a clean signal with some noise in the baseline.

Ch 3 is a clean signal with some noise in the baseline.

  
30141 09/10/13

30141_0.5_0.data

30141_0.5_1.data

30141_0.5_2.data

30141_0.5_3.data

 Pierre            
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre            
>
>
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~0.68 V) at 0.069 sec and has no other peaks larger than 0.26 V. This channel also has high frequency signals that are disgused within particle peaks. Zoom in to differentiate.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has decently clean with good peaks but some noise embedded in the baseline signal.

Ch 3 has a clean signal

  
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a grouping of high frequency noise (~0.60 V) at 0.387 sec alongside not having any particle peaks above 0.25 V.

Ch 1 has a clean signal with good peak shapes.

Ch 2 has a clean signal with some noise in the baseline but the peaks are consistent.

Ch 3 has a large peak (~2.70 V) at 0.246 sec and prevalent noise in the baseline but otherwise clean good peaks.

  
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.27 V and has a lot of noise that peaks inconsistent in shape.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has a clean signal with some noise in the baseline.

Ch 3 has a clean signal with some noise in the baseline.

  
30141 09/10/13

30141_0.5_0.data

30141_0.5_1.data

30141_0.5_2.data

30141_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.26 V with very noisy peaks.

Ch 1 has a clean signal with consistent peak shapes.

Ch 2 has some noise but otherwise clean, consistent peaks.

Ch 3 has a clean signal with good peaks.

  
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is riddled with so much noise that most peaks are impossible to distinguish from noise.

Ch 1 has a large reflected peak (~ -3.31 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 2 has a large reflected peak (~ -3.04 V) at 0.440 sec but otherwise has clean consistent peaks.

Ch 3 has a large reflected peak (~ -2.67 V) at 0.440 sec but otherwise has clean consistent peaks.

  
 
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre            
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre            
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre            

Revision 922014-07-09 - clope023

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 229 to 229
 
30047 09/04/13

30047_0.5_0.data

30047_0.5_1.data

30047_0.5_2.data

30047_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30048 09/04/13

30048_0.5_0.data

30048_0.5_1.data

30048_0.5_2.data

30048_0.5_3.data

 Omar No yes Yes Yes Channel 0 has very noisy peaks.  
30049 09/04/13

30049_0.5_0.data

30049_0.5_1.data

30049_0.5_2.data

30049_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
Changed:
<
<
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck

  
30051                  
30052                  
30053                  
30054                  
30055                  
30056                  
30057                  
30058                  
30059                  
30060                  
30062                  
30063                  
30064                  
30065                  
30066                  
30067                  
30068                  
30069                  
30071                  
30073                  
30074                  
30075                  
30076                  
30077                  
>
>
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Lopez Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck

  
30051 09/05/2013

30051_0.5_0.data

30051_0.5_1.data

30051_0.5_2.data

30051_0.5_3.data

 Carlos Lopez No No No No

Ch0: nothing/noisy

Ch1: noisy

Ch2: noisy

Ch3: noisy

  
30052 09/05/2013

30052_0.5_0.data

30052_0.5_1.data

30052_0.5_2.data

30052_0.5_3.data

 Carlos Lopez No No No No Noise in all channels  
30053 09/05/2013

30053_0.5_0.data

30053_0.5_1.data

30053_0.5_2.data

30053_0.5_3.data 		Carlos Lopez No Yes Yes Yes Ch0: noise  
30054 09/05/2013

30054_0.5_0.data

30054_0.5_1.data

30054_0.5_2.data

30054_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30055 09/05/2013

30055_0.5_0.data

30055_0.5_1.data

30055_0.5_2.data

30055_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30056 09/05/2013

30056_0.5_0.data

30056_0.5_1.data

30056_0.5_2.data

30056_0.5_3.data

 Carlos Lopez No No No No All channels had too much noise  
30057 09/05/2013 30057_0.5_0.data

30057_0.5_1.data

30057_0.5_2.data

30057_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30058 09/05/2013 30058_0.5_0.data

30058_0.5_1.data

30058_0.5_2.data

30058_0.5_3.data 		Carlos Lopez No No No No Noise in all channels  
30059 09/05/2013

30059_0.5_0.data

30059_0.5_1.data

30059_0.5_2.data

30059_0.5_3.data

 Carlos Lopez No No No No Noise in all channels  
30060 09/05/2013

30060_0.5_0.data

30060_0.5_1.data

30060_0.5_2.data

30060_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30062 09/05/2013

30062_0.5_0.data

30062_0.5_1.data

30062_0.5_2.data

30062_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30063 09/05/2013

30063_0.5_0.data

30063_0.5_1.data

30063_0.5_2.data

30063_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30064 09/05/2013

30064_0.5_0.data

30064_0.5_1.data

30064_0.5_2.data

30064_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30065 09/05/2013

30065_0.5_0.data

30065_0.5_1.data

30065_0.5_2.data

30065_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch0: noise  
30066 09/05/2013

30066_0.5_0.data

30066_0.5_1.data

30066_0.5_2.data

30066_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30067 09/05/2013

30067_0.5_0.data

30067_0.5_1.data

30067_0.5_2.data

30067_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30068 09/05/2013

30068_0.5_0.data

30068_0.5_1.data

30068_0.5_2.data

30068_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30069 09/05/2013

30069_0.5_0.data

30069_0.5_1.data

30069_0.5_2.data

30069_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30071 09/05/2013

30071_0.5_0.data

30071_0.5_1.data

30071_0.5_2.data

30071_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30073 09/05/2013

30073_0.5_0.data

30073_0.5_1.data

30073_0.5_2.data

30073_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30074 09/05/2013

30074_0.5_0.data

30074_0.5_1.data

30074_0.5_2.data

30074_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30075 09/05/2013

30075_0.5_0.data

30075_0.5_1.data

30075_0.5_2.data

30075_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30076 09/05/2013

30076_0.5_0.data

30076_0.5_1.data

30076_0.5_2.data

30076_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
30077 09/05/2013

30077_0.5_0.data

30077_0.5_1.data

30077_0.5_2.data

30077_0.5_3.data

 Carlos Lopez No Yes Yes Yes Ch 0: noise  
 
30078                  
30079                  
30080                  

Revision 912014-07-08 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 313 to 313
 
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

Ch 2 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. The baseline signal is somewhat noisy but a mojority of paritcle peaks have clean shapes.

Ch 3 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. This channel also has gaps of no activity but other than that is clean and had good peaks.

  
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~0.68 V) at 0.069 sec and has no other peaks larger than 0.26 V. This channel also has high frequency signals that are disgused within particle peaks. Zoom in to differentiate.

Ch 1 is a clean signal with consistent peak shapes.

Ch 2 is decently clean with good peaks but some noise embedded in the baseline signal.

Ch 3 is a clean signal

  
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a grouping of high frequency noise (~0.60 V) at 0.387 sec alongside not having any particle peaks above 0.25 V.

Ch 1 is a clean signal with good peak shapes.

Ch 2 is a clean signal with some noise in the baseline but the peaks are consistent.

Ch 3 has a large peak (~2.70 V) at 0.246 sec and prevelant noise in the baseline but otherwise clean good peaks.

  
Changed:
<
<
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre            
30141                  
30142                  
30143                  
30144                  
30145                  
>
>
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has no peaks higher than 0.27 V and has a lot of noise that peaks inconsistent in shape.

Ch 1 is a clean signal with consistent peak shapes.

Ch 2 is a clean signal with some noise in the baseline.

Ch 3 is a clean signal with some noise in the baseline.

  
30141 09/10/13

30141_0.5_0.data

30141_0.5_1.data

30141_0.5_2.data

30141_0.5_3.data

 Pierre            
30142 09/10/13

30142_0.5_0.data

30142_0.5_1.data

30142_0.5_2.data

30142_0.5_3.data

 Pierre            
30143 09/10/13

30143_0.5_0.data

30143_0.5_1.data

30143_0.5_2.data

30143_0.5_3.data

 Pierre            
30144 09/10/13

30144_0.5_0.data

30144_0.5_1.data

30144_0.5_2.data

30144_0.5_3.data

 Pierre            
30145 09/10/13

30145_0.5_0.data

30145_0.5_1.data

30145_0.5_2.data

30145_0.5_3.data

 Pierre            
 
30147                  
30148                  
30149                  

Revision 902014-07-08 - jlatorre1513

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 195 to 195
 
29980 08/22/13

29980_0.5_0.data

29980_0.5_1.data

29980_0.5_2.data

29980_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .3s, everything afterwards is just noise  
29981 08/22/13

29981_0.5_0.data

29981_0.5_1.data

29981_0.5_2.data

29981_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .33s, everything afterwards is just noise  
29982 08/22/13

29982_0.5_0.data

29982_0.5_1.data

29982_0.5_2.data

29982_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .35s. Each one had a last voltage peak at around t = .351s with a v = 3.4  
Changed:
<
<
29983 08/22/13

29983_0.5_0.data

29983_0.5_1.data

29983_0.5_2.data

29983_0.5_3.data

 Javiera            
29984 08/22/13

29984_0.5_0.data

29984_0.5_1.data

29984_0.5_2.data

29984_0.5_3.data

 Javiera            
>
>
29983 08/22/13

29983_0.5_0.data

29983_0.5_1.data

29983_0.5_2.data

29983_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: All of these are useful between t = .05s to t = .35s. In each one there is a large voltage peak at around t - .35s with a voltage of about 3.4V  
29984 08/22/13

29984_0.5_0.data

29984_0.5_1.data

29984_0.5_2.data

29984_0.5_3.data

 Javiera No No No No These channels were mostly, if not all, noise.  
 
29985                  
29986                  
29987                  

Revision 892014-07-07 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 311 to 311
 
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
30136 09/10/13

30136_0.5_0.data

30136_0.5_1.data

30136_0.5_2.data

30136_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large peaks at 0.209 and 0.300 sec (~1.0 V) and a noise peak (~1.0 V) at 0.500 sec. The peaks in this channel are drowned with noise and are inconsistent in shape.

Ch 1 has a few sections of over saturated signals from 0.190 to 0.309 sec.

Ch 2 has a noisy baseline but the peaks are consistent in shape.

Ch 3 has a clean signal.

  
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

Ch 2 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. The baseline signal is somewhat noisy but a mojority of paritcle peaks have clean shapes.

Ch 3 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. This channel also has gaps of no activity but other than that is clean and had good peaks.

  
Changed:
<
<
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre            
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre            
>
>
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~0.68 V) at 0.069 sec and has no other peaks larger than 0.26 V. This channel also has high frequency signals that are disgused within particle peaks. Zoom in to differentiate.

Ch 1 is a clean signal with consistent peak shapes.

Ch 2 is decently clean with good peaks but some noise embedded in the baseline signal.

Ch 3 is a clean signal

 
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a grouping of high frequency noise (~0.60 V) at 0.387 sec alongside not having any particle peaks above 0.25 V.

Ch 1 is a clean signal with good peak shapes.

Ch 2 is a clean signal with some noise in the baseline but the peaks are consistent.

Ch 3 has a large peak (~2.70 V) at 0.246 sec and prevelant noise in the baseline but otherwise clean good peaks.

 
 
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre            
30141                  
30142                  

Revision 882014-07-03 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 310 to 310
 
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
30136 09/10/13

30136_0.5_0.data

30136_0.5_1.data

30136_0.5_2.data

30136_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large peaks at 0.209 and 0.300 sec (~1.0 V) and a noise peak (~1.0 V) at 0.500 sec. The peaks in this channel are drowned with noise and are inconsistent in shape.

Ch 1 has a few sections of over saturated signals from 0.190 to 0.309 sec.

Ch 2 has a noisy baseline but the peaks are consistent in shape.

Ch 3 has a clean signal.

  
Changed:
<
<
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes    

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

  
>
>
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

Ch 2 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. The baseline signal is somewhat noisy but a mojority of paritcle peaks have clean shapes.

Ch 3 has large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, and 0.448. This channel also has gaps of no activity but other than that is clean and had good peaks.

  
 
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre            
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre            
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre            

Revision 872014-07-03 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 310 to 310
 
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
30136 09/10/13

30136_0.5_0.data

30136_0.5_1.data

30136_0.5_2.data

30136_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large peaks at 0.209 and 0.300 sec (~1.0 V) and a noise peak (~1.0 V) at 0.500 sec. The peaks in this channel are drowned with noise and are inconsistent in shape.

Ch 1 has a few sections of oversaturated signals from 0.190 to 0.309 sec.

Ch 2 has a noisy baseline but the peaks are consistent in shape.

Ch 3 has a clean signal.

  
Changed:
<
<
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre            
>
>
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre No Yes    

Ch 0 has no peaks larger 0.3 V save for noise peaks (~3.0 V). Peaks are very inconsistent in shape and filled with noise.

Ch 1 has the same large noise peaks (~3.0 V) at 0.270, 0.360, 0.385, 0.448, and a smaller noise peak at 0.408.

  
 
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre            
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre            
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre            

Revision 862014-07-03 - jlatorre1513

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 194 to 194
 
29978 08/22/13

29978_0.5_0.data

29978_0.5_1.data

29978_0.5_2.data

29978_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .3s, everything afterwards is just noise  
29980 08/22/13

29980_0.5_0.data

29980_0.5_1.data

29980_0.5_2.data

29980_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .3s, everything afterwards is just noise  
29981 08/22/13

29981_0.5_0.data

29981_0.5_1.data

29981_0.5_2.data

29981_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .33s, everything afterwards is just noise  
Changed:
<
<
29982 08/22/13

29982_0.5_0.data

29982_0.5_1.data

29982_0.5_2.data

29982_0.5_3.data

 Javiera            
>
>
29982 08/22/13

29982_0.5_0.data

29982_0.5_1.data

29982_0.5_2.data

29982_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .35s. Each one had a last voltage peak at around t = .351s with a v = 3.4  
 
29983 08/22/13

29983_0.5_0.data

29983_0.5_1.data

29983_0.5_2.data

29983_0.5_3.data

 Javiera            
29984 08/22/13

29984_0.5_0.data

29984_0.5_1.data

29984_0.5_2.data

29984_0.5_3.data

 Javiera            
29985                  

Revision 852014-07-03 - jlatorre1513

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 186 to 186
 
29966 08/22/13   Ramona No Yes Yes Yes    
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise

  
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s

  
Changed:
<
<
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s  
>
>
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

29971_0.5_2.data

29971_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful between t = .100s to t = .310s  
 
29972 08/22/13   Ramona No Yes Yes Yes    
Changed:
<
<
29974                  
29975     Ramona No Yes Yes Yes    
29976     Ramona No Yes Yes Yes    
29978                  
29980     Ramona No Yes Yes Yes    
29981                  
29982                  
29983                  
29984                  
>
>
29974 08/22/13

29974_0.5_0.data

29974_0.5_1.data

29974_0.5_2.data

29974_0.5_3.data

 Javiera No No No No Every channel was only noise  
29975 08/22/13

29975_0.5_0.data

29975_0.5_1.data

29975_0.5_2.data

29975_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch2, Ch3: Most useful between t = .1s to t = .3s  
29976 08/22/13

29976_0.5_0.data

29976_0.5_1.data

29976_0.5_2.data

29976_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Most useful between t = .1s to t = .27s  
29978 08/22/13

29978_0.5_0.data

29978_0.5_1.data

29978_0.5_2.data

29978_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = .05s to t = .3s, everything afterwards is just noise  
29980 08/22/13

29980_0.5_0.data

29980_0.5_1.data

29980_0.5_2.data

29980_0.5_3.data

 Ramona/ Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .3s, everything afterwards is just noise  
29981 08/22/13

29981_0.5_0.data

29981_0.5_1.data

29981_0.5_2.data

29981_0.5_3.data

 Javiera No Yes Yes Yes Ch1, Ch2, Ch3: Useful from t = 0s to t = .33s, everything afterwards is just noise  
29982 08/22/13

29982_0.5_0.data

29982_0.5_1.data

29982_0.5_2.data

29982_0.5_3.data

 Javiera            
29983 08/22/13

29983_0.5_0.data

29983_0.5_1.data

29983_0.5_2.data

29983_0.5_3.data

 Javiera            
29984 08/22/13

29984_0.5_0.data

29984_0.5_1.data

29984_0.5_2.data

29984_0.5_3.data

 Javiera            
 
29985                  
29986                  
29987                  

Revision 842014-07-02 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 309 to 309
 
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has some noise, particularly many reflected peaks throughout the shot. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 is a much cleaner signal than Ch 0. Peaks are consistent.

Ch 2 has a noisy baseline but good peaks.

Ch 3 also has a noisy baseline but the peaks are good.

  
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
Changed:
<
<
30136                  
30137                  
30138                  
30139                  
30140                  
>
>
30136 09/10/13

30136_0.5_0.data

30136_0.5_1.data

30136_0.5_2.data

30136_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large peaks at 0.209 and 0.300 sec (~1.0 V) and a noise peak (~1.0 V) at 0.500 sec. The peaks in this channel are drowned with noise and are inconsistent in shape.

Ch 1 has a few sections of oversaturated signals from 0.190 to 0.309 sec.

Ch 2 has a noisy baseline but the peaks are consistent in shape.

Ch 3 has a clean signal.

  
30137 09/10/13

30137_0.5_0.data

30137_0.5_1.data

30137_0.5_2.data

30137_0.5_3.data

 Pierre            
30138 09/10/13

30138_0.5_0.data

30138_0.5_1.data

30138_0.5_2.data

30138_0.5_3.data

 Pierre            
30139 09/10/13

30139_0.5_0.data

30139_0.5_1.data

30139_0.5_2.data

30139_0.5_3.data

 Pierre            
30140 09/10/13

30140_0.5_0.data

30140_0.5_1.data

30140_0.5_2.data

30140_0.5_3.data

 Pierre            
 
30141                  
30142                  
30143                  

Revision 832014-06-21 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 352 to 352
 
30178                  
30179                  
30180 09/12/13

30180_0.5_0.data

30180_0.5_1.data

30180_0.5_2.data

30180_0.5_3.data

 Omar No No No No All four channels were composed of noise.  
Changed:
<
<
30181                  
30182                  
30183                  
30184                  
30185                  
30187                  
>
>
30181 09/12/13

30181_0.5_0.data

30181_0.5_1.data

30181_0.5_2.data

30181_0.5_3.data

Omar No No No No All channels are composed of noise.  
30182 09/12/13

30182_0.5_0.data

30182_0.5_1.data

30182_0.5_2.data

30182_0.5_3.data

Omar No Yes Yes Yes Channel 0 has very noisy peaks. Channel 1 has a sharp decrease in data at ~.35s.  
30183 09/12/13

30183_0.5_0.data

30183_0.5_1.data

30183_0.5_2.data

30183_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30184 09/12/13

30184_0.5_0.data

30184_0.5_1.data

30184_0.5_2.data

30184_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30185 09/12/13

30185_0.5_0.data

30185_0.5_1.data

30185_0.5_2.data

30185_0.5_3.data

Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30187 09/12/13

30187_0.5_0.data

30187_0.5_1.data

30187_0.5_2.data

30187_0.5_3.data

Omar No Yes Yes Yes Channel 0 has very noisy peaks. All other channels have a sharp decrease in data at ~.29s.  
 
30188                  
30189                  
30190                  

Revision 822014-06-19 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 308 to 308
 
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has some noise, particularly many reflected peaks throughout the shot. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 is a much cleaner signal than Ch 0. Peaks are consistent.

Ch 2 has a noisy baseline but good peaks.

Ch 3 also has a noisy baseline but the peaks are good.

  
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
Changed:
<
<
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No      

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

  
>
>
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

Ch 2 has a clean signal, occasional shifts in baseline, may lead to high rates.

Ch 3 has a clean signal with consistent peaks.

  
 
30136                  
30137                  
30138                  

Revision 812014-06-19 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 308 to 308
 
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has some noise, particularly many reflected peaks throughout the shot. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 is a much cleaner signal than Ch 0. Peaks are consistent.

Ch 2 has a noisy baseline but good peaks.

Ch 3 also has a noisy baseline but the peaks are good.

  
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
Changed:
<
<
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No      

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

  
>
>
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No      

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

Ch 1 has a handful of reflected peaks from 0.200 to 0.250 sec.

  
 
30136                  
30137                  
30138                  

Revision 802014-06-18 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 307 to 307
 
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few small reflected peaks but is otherwise relatively free of noise.

Ch 1 has a few small reflected peaks but is also clean.

Ch 2 has a noisy baseline.

Ch 3 has a clean signal.

  
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has some noise, particularly many reflected peaks throughout the shot. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 is a much cleaner signal than Ch 0. Peaks are consistent.

Ch 2 has a noisy baseline but good peaks.

Ch 3 also has a noisy baseline but the peaks are good.

  
Changed:
<
<
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes    

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

  
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre            
>
>
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

Ch 2 has a large peak (~ 1.5 V) at 0.325 sec. Noisy baseline but peaks are consistent.

Ch 3 has a noisy baseline but peaks are consistent.

  
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre No      

Ch 0 has a large peak (~ 1.2 V) at 0.229 sec, 2 high freq noise peak (~ 0.75, 0.66 V) at 0.236 and 0.401 sec. There is too much noise in peaks and variations in shape.

  
 
30136                  
30137                  
30138                  

Revision 792014-06-18 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Changed:
<
<

Back to MAST Diagnostic

>
>

Back to MAST Diagnostic

 
Changed:
<
<

Detector Orientations

>
>

Detector Orientations

 

Data Channel #

Detector Positions

Angular Orientation

Trajectory Color

Detector Collimator Entrance Offset from RP
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm
Line: 23 to 24
  Figure Set 4: Detector Angular Orientations

Changed:
<
<
Data Log
>
>
Plasma Scenarios
 
Deleted:
<
<		Scenario Shots
 
Scenario: Reference Shots

     
Beam Blip/ NBI Slowing Down 29958 29960 29966 29972 - -
Quiescent MHD 29904 29905 29906 29908 29909 29910
Line: 37 to 37
 
Scenario: Non-Resonant Perturbations Shots

       
Sawteeth 29879 29880 29881 29882 29883 29884 29885
Changed:
<
<

Shot Log

>
>

Shot Log

 
Shot Date
080513
081613

Revision 782014-06-17 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 12 to 12
 
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3
Changed:
<
<
  • Note that for the shot_list.data on nyoko2, the setpoint values are the input values to the RP control box during data collection
>
>		Note that for the shot_list.data on nyoko2, the setpoint values are the input values to the RP control box during data collection
 Figure Set 1: Detector Positions

Figure Set 2: Channel Particle Trajectories

Line: 300 to 301
 
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -0.8 V) at 0.177 sec.

Ch 1 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 2 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 3 has a good signal with little noise.

  
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak at 0.290 sec.

Ch 1 has a large reflected peak (~ -3.35 V) at 0.290 sec.

Ch 2 has a large reflected peak (~ -3.30 V) at 0.290 sec.

Ch 3 has a large reflected peak (~ -2.65 V) at 0.290 sec.

  
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few small reflected peaks but is otherwise relatively free of noise.

Ch 1 has a few small reflected peaks but is also clean.

Ch 2 has a noisy baseline.

Ch 3 has a clean signal.

  
Changed:
<
<
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre            
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre            
>
>
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has some noise, particularly many reflected peaks throughout the shot. Later in the shot peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 is a much cleaner signal than Ch 0. Peaks are consistent.

Ch 2 has a noisy baseline but good peaks.

Ch 3 also has a noisy baseline but the peaks are good.

  
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre Yes Yes    

Ch 0 has a large peak (~ 2.25 V) at 0.325 sec. Hardly any peaks exceed 0.5 V in height and are inconsistent in shape.

Ch 1 has two large peaks (~ 2.0 V, 1.8 V) at 0.325 and 0.360 sec. Peaks are cleaner but occasionally have noise oscillations disturbing their shape.

  
 
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre            
30136                  
30137                  

Revision 772014-06-17 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 299 to 299
 
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a clean signal with little noise and consistent peaks.

Ch 1 has a large reflected peak at 0.360 sec.

Ch 2 has a large reflected peak at 0.360 sec.

Ch 3 has a large reflected peak at 0.359 sec.

  
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -0.8 V) at 0.177 sec.

Ch 1 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 2 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 3 has a good signal with little noise.

  
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak at 0.290 sec.

Ch 1 has a large reflected peak (~ -3.35 V) at 0.290 sec.

Ch 2 has a large reflected peak (~ -3.30 V) at 0.290 sec.

Ch 3 has a large reflected peak (~ -2.65 V) at 0.290 sec.

  
Changed:
<
<
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few small reflected peaks but is otherwise realtively free of noise.

Ch 1 has a few small reflected peaks but is also clean.

Ch 2 has a noisy baseline.

Ch 3 has a clean signal.

  
30132                  
30133                  
30134                  
30135                  
>
>
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few small reflected peaks but is otherwise relatively free of noise.

Ch 1 has a few small reflected peaks but is also clean.

Ch 2 has a noisy baseline.

Ch 3 has a clean signal.

  
30132 09/10/13

30132_0.5_0.data

30132_0.5_1.data

30132_0.5_2.data

30132_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large noise peak (~ 3.5 V) at 0.441 sec. Peaks are irregular and a majority do not exceed 0.3 V in height.

Ch 1 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 2 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

Ch 3 has a large noise peak (~ 3.5 V) at 0.441 sec and at 0.445 sec. Peaks are consistent in shape and height.

  
30133 09/10/13

30133_0.5_0.data

30133_0.5_1.data

30133_0.5_2.data

30133_0.5_3.data

 Pierre            
30134 09/10/13

30134_0.5_0.data

30134_0.5_1.data

30134_0.5_2.data

30134_0.5_3.data

 Pierre            
30135 09/10/13

30135_0.5_0.data

30135_0.5_1.data

30135_0.5_2.data

30135_0.5_3.data

 Pierre            
 
30136                  
30137                  
30138                  

Revision 762014-06-16 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 299 to 299
 
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a clean signal with little noise and consistent peaks.

Ch 1 has a large reflected peak at 0.360 sec.

Ch 2 has a large reflected peak at 0.360 sec.

Ch 3 has a large reflected peak at 0.359 sec.

  
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -0.8 V) at 0.177 sec.

Ch 1 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 2 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 3 has a good signal with little noise.

  
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak at 0.290 sec.

Ch 1 has a large reflected peak (~ -3.35 V) at 0.290 sec.

Ch 2 has a large reflected peak (~ -3.30 V) at 0.290 sec.

Ch 3 has a large reflected peak (~ -2.65 V) at 0.290 sec.

  
Changed:
<
<
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre            
>
>
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few small reflected peaks but is otherwise realtively free of noise.

Ch 1 has a few small reflected peaks but is also clean.

Ch 2 has a noisy baseline.

Ch 3 has a clean signal.

  
 
30132                  
30133                  
30134                  

Revision 752014-06-16 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 298 to 298
 
30126 09/10/13

30126_0.5_0.data

30126_0.5_1.data

30126_0.5_2.data

30126_0.5_3.data

 Pierre No No No No

Ch 2 contains only high frequency noise (~ Amplitude 0.2 V)

Ch3 same as latter.

  
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a clean signal with little noise and consistent peaks.

Ch 1 has a large reflected peak at 0.360 sec.

Ch 2 has a large reflected peak at 0.360 sec.

Ch 3 has a large reflected peak at 0.359 sec.

  
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -0.8 V) at 0.177 sec.

Ch 1 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 2 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 3 has a good signal with little noise.

  
Changed:
<
<
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre            
>
>
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak at 0.290 sec.

Ch 1 has a large reflected peak (~ -3.35 V) at 0.290 sec.

Ch 2 has a large reflected peak (~ -3.30 V) at 0.290 sec.

Ch 3 has a large reflected peak (~ -2.65 V) at 0.290 sec.

  
 
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre            
30132                  
30133                  

Revision 742014-06-13 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 147 to 147
 
29930 08/20/13   Douglas No No No No All channels mostly noise.  
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes    
29932                  
Changed:
<
<
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise  
>
>
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera/Omar No No No No Every channel was only noise  
 
29934                  
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes    
29936                  
Line: 346 to 346
 
30177                  
30178                  
30179                  
Changed:
<
<
30180                  
>
>
30180 09/12/13

30180_0.5_0.data

30180_0.5_1.data

30180_0.5_2.data

30180_0.5_3.data

 Omar No No No No All four channels were composed of noise.  
 
30181                  
30182                  
30183                  

Revision 732014-06-13 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 220 to 220
 
30042 09/04/13

30042_0.5_0.data

30042_0.5_1.data

30042_0.5_2.data

30042_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.  
30043 09/04/13

30043_0.5_0.data

30043_0.5_1.data

30043_0.5_2.data

30043_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .24 seconds.  
30044 09/04/13

30044_0.5_0.data

30044_0.5_1.data

30044_0.5_2.data

30044_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .36 seconds.  
Changed:
<
<
30045                  
30047                  
30048                  
30049                  
>
>
30045 09/04/13

30045_0.5_0.data

30045_0.5_1.data

30045_0.5_2.data

30045_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30047 09/04/13

30047_0.5_0.data

30047_0.5_1.data

30047_0.5_2.data

30047_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
30048 09/04/13

30048_0.5_0.data

30048_0.5_1.data

30048_0.5_2.data

30048_0.5_3.data

 Omar No yes Yes Yes Channel 0 has very noisy peaks.  
30049 09/04/13

30049_0.5_0.data

30049_0.5_1.data

30049_0.5_2.data

30049_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has very noisy peaks.  
 
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck

  
30051                  
30052                  

Revision 722014-06-13 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 297 to 297
 
30125 09/10/13

30125_0.5_0.data

30125_0.5_1.data

30125_0.5_2.data

30125_0.5_3.data

 Pierre No No No No There are no particle peaks in any channels.  
30126 09/10/13

30126_0.5_0.data

30126_0.5_1.data

30126_0.5_2.data

30126_0.5_3.data

 Pierre No No No No

Ch 2 contains only high frequency noise (~ Amplitude 0.2 V)

Ch3 same as latter.

  
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a clean signal with little noise and consistent peaks.

Ch 1 has a large reflected peak at 0.360 sec.

Ch 2 has a large reflected peak at 0.360 sec.

Ch 3 has a large reflected peak at 0.359 sec.

  
Changed:
<
<
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre            
>
>
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -0.8 V) at 0.177 sec.

Ch 1 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 2 has a large reflected peak (~ -0.8 V) at 0.210 sec.

Ch 3 has a good signal with little noise.

  
 
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre            
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre            
30132                  

Revision 712014-06-12 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 296 to 296
 
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy and peaks are erratic.

Ch 1 is clean with a few gaps of flatline signal.

Ch 2 is a decently clean with a noisy baseline.

Ch 3 is decently clean with a noisy baseline and many particle peaks with large amplitudes (~ 1.5 V)

  
30125 09/10/13

30125_0.5_0.data

30125_0.5_1.data

30125_0.5_2.data

30125_0.5_3.data

 Pierre No No No No There are no particle peaks in any channels.  
30126 09/10/13

30126_0.5_0.data

30126_0.5_1.data

30126_0.5_2.data

30126_0.5_3.data

 Pierre No No No No

Ch 2 contains only high frequency noise (~ Amplitude 0.2 V)

Ch3 same as latter.

  
Changed:
<
<
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes       Ch 0 is a clean signal with little noise and consistent peaks.  
>
>
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 is a clean signal with little noise and consistent peaks.

Ch 1 has a large reflected peak at 0.360 sec.

Ch 2 has a large reflected peak at 0.360 sec.

Ch 3 has a large reflected peak at 0.359 sec.

  
 
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre            
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre            
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre            

Revision 702014-06-12 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 294 to 294
 
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has quite a few reflected peaks and a large noise peak at 0.211 sec. There is a lot of low voltage noise embedded in the baseline signal.

Ch 1 is a cleaner signal than Ch 0 with a few reflected noise peaks.

Ch 2 is a cleaner signal than Ch 0 but with a noiser baseline signal.

Ch 3 is a cleaner signal than Ch 0 but with a noiser baseline signal.

  
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few reflected peaks and a noisy baseline near the middle of the shot.

Ch 1 has a clean signal.

Ch 2 has a very clean signal.

Ch 3 has a clean signal.

  
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy and peaks are erratic.

Ch 1 is clean with a few gaps of flatline signal.

Ch 2 is a decently clean with a noisy baseline.

Ch 3 is decently clean with a noisy baseline and many particle peaks with large amplitudes (~ 1.5 V)

  
Changed:
<
<
30125                  
30126                  
30127                  
30128                  
30130                  
30131                  
>
>
30125 09/10/13

30125_0.5_0.data

30125_0.5_1.data

30125_0.5_2.data

30125_0.5_3.data

 Pierre No No No No There are no particle peaks in any channels.  
30126 09/10/13

30126_0.5_0.data

30126_0.5_1.data

30126_0.5_2.data

30126_0.5_3.data

 Pierre No No No No

Ch 2 contains only high frequency noise (~ Amplitude 0.2 V)

Ch3 same as latter.

  
30127 09/10/13

30127_0.5_0.data

30127_0.5_1.data

30127_0.5_2.data

30127_0.5_3.data

 Pierre Yes       Ch 0 is a clean signal with little noise and consistent peaks.  
30128 09/10/13

30128_0.5_0.data

30128_0.5_1.data

30128_0.5_2.data

30128_0.5_3.data

 Pierre            
30130 09/10/13

30130_0.5_0.data

30130_0.5_1.data

30130_0.5_2.data

30130_0.5_3.data

 Pierre            
30131 09/10/13

30131_0.5_0.data

30131_0.5_1.data

30131_0.5_2.data

30131_0.5_3.data

 Pierre            
 
30132                  
30133                  
30134                  

Revision 692014-06-11 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 292 to 292
 
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.

  
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy with a few large high frequency waves of large amplitudes.

Ch 1 is considerably cleaner with only one large amplitude high frequency noise peak at 0.212 sec.

Ch 2 is also clean with a single large amplitude high frequency noise peak.

Ch 3 is a clean signal with a single large amplitude high frequency noise peak at 0.213 sec.

  
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has quite a few reflected peaks and a large noise peak at 0.211 sec. There is a lot of low voltage noise embedded in the baseline signal.

Ch 1 is a cleaner signal than Ch 0 with a few reflected noise peaks.

Ch 2 is a cleaner signal than Ch 0 but with a noiser baseline signal.

Ch 3 is a cleaner signal than Ch 0 but with a noiser baseline signal.

  
Changed:
<
<
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few reflected peaks and a noisey baseline near the middle of the shot.

Ch 1 has a clean signal.

Ch 2 has a very clean signal.

Ch 3 has a clean signal.

  
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre            
>
>
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few reflected peaks and a noisy baseline near the middle of the shot.

Ch 1 has a clean signal.

Ch 2 has a very clean signal.

Ch 3 has a clean signal.

  
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy and peaks are erratic.

Ch 1 is clean with a few gaps of flatline signal.

Ch 2 is a decently clean with a noisy baseline.

Ch 3 is decently clean with a noisy baseline and many particle peaks with large amplitudes (~ 1.5 V)

  
 
30125                  
30126                  
30127                  

Revision 682014-06-10 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 292 to 292
 
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.

  
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy with a few large high frequency waves of large amplitudes.

Ch 1 is considerably cleaner with only one large amplitude high frequency noise peak at 0.212 sec.

Ch 2 is also clean with a single large amplitude high frequency noise peak.

Ch 3 is a clean signal with a single large amplitude high frequency noise peak at 0.213 sec.

  
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has quite a few reflected peaks and a large noise peak at 0.211 sec. There is a lot of low voltage noise embedded in the baseline signal.

Ch 1 is a cleaner signal than Ch 0 with a few reflected noise peaks.

Ch 2 is a cleaner signal than Ch 0 but with a noiser baseline signal.

Ch 3 is a cleaner signal than Ch 0 but with a noiser baseline signal.

  
Changed:
<
<
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre            
>
>
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a few reflected peaks and a noisey baseline near the middle of the shot.

Ch 1 has a clean signal.

Ch 2 has a very clean signal.

Ch 3 has a clean signal.

  
 
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre            
30125                  
30126                  

Revision 672014-06-09 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 54 to 54
 
091213

Yes

Changed:
<
<
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

   No Yes      
29807                
29808                
29809                
29811                
29812                
29813                
29814                
29815                
29818                
29820                
29821                
29822                
29823                
29824                
29825                
29826                
29827                
29828                
29829                
29832                
29834                
29835                
29837                
29838                
29839                
29840                
29841                
29845                
29846                
29847                
29848                
29849                
29851                
29852                
29853                
29854                
29855                
29859                
29862                
29874                
29875                
29876                
29877                
29878                
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes  
29880 08/19/13   Werner/ Ramona Yes No Yes Yes  
29881 08/19/13   Werner/ Ramona No Yes Yes Yes  
29882 08/19/13   Werner/ Ramona Yes No Yes Yes  
29883     Werner/ Ramona Yes Yes Yes Yes  
29884     Werner/ Ramona Yes Yes Yes Yes  
29885     Werner/ Ramona Yes Yes Yes Yes  
29890                
29891                
29892                
29893                
29894                
29895                
29896                
29897                
29898                
29899 08/20/13   Douglas No No No No All channels only noise.
29901 08/20/13   Douglas No No No No All channels only noise.
29902 08/20/13   Douglas No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.
29904 08/20/13   Pierre/ Ramona No No No No  
29905 08/20/13   Pierre/ Ramona No No No No  
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Omar/ Ramona

Douglas

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise
29907 08/20/13

29907_0.5_0.data

29907_0.5_1.data

29907_0.5_2.data

29907_0.5_3.data

 Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13

29908_0.5_0.data

29908_0.5_2.data

29908_0.5_3.data

Pierre

Douglas

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.
29909 08/20/13

29909_0.5_0.data

29909_0.5_1.data

29909_0.5_2.data

29909_0.5_3.data

 Ramona/ Pierre Yes Yes Yes Yes  
29910 08/20/13

29910_0.5_1.data

29910_0.5_2.data

29910_0.5_3.data

 Ramona/ Pierre No Yes Yes Yes  
29911 08/20/13   Douglas No No No No  
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

 Douglas No Yes Yes Yes  
29914 08/20/13

29914_0.5_1.data

29914_0.5_2.data

29914_0.5_3.data

 Douglas No Yes Yes Yes  
29915 08/20/13

29915_0.5_1.data

29915_0.5_2.data

29915_0.5_3.data

 Douglas No Yes Yes Yes  
29916 08/20/13   Douglas No No No No  
29917 08/20/13

29917_0.5_1.data

29917_0.5_2.data

29917_0.5_3.data

 Ramona No Yes Yes Yes  
29918 08/20/13   Douglas No No No No  
29919 08/2013

29919_0.5_1.data

29919_0.5_2.data

29919_0.5_3.data

Douglas

 No Yes Yes Yes  
29920 08/20/13

29920_0.5_1.data

29920_0.5_2.data

29920_0.5_3.data

Werner

Douglas

 No Yes Yes Yes  
29921 08/20/13

29921_0.5_2.data

29921_0.5_3.data

 Douglas No No Yes Yes  
29922 08/20/13

29922_0.5_1.data

29922_0.5_2.data

29922_0.5_3.data

 Douglas No Yes Yes Yes  
29923 08/20/13

29923_0.5_1.data

29923_0.5_2.data

29923_0.5_3.data

 Douglas No Yes Yes Yes  
29924 08/20/13

29924_0.5_0.data

29924_0.5_1.data

29924_0.5_2.data

29924_0.5_3.data

Ramona/ Omar

Douglas

 No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925 08/20/13

29925_0.5_1.data

29925_0.5_2.data

29925_0.5_3.data

 Douglas No Yes Yes Yes  
29926 08/20/13   Douglas No No No No  
29927 08/20/13   Douglas No No No No  
29928 08/20/13   Ramona No Yes Yes Yes  
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
29930 08/20/13   Douglas No No No No All channels mostly noise.
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
29932                
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
29934                
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes  
29936                
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes  
29938                
29939                
29940                
29941                
29942                
29943                
29944                
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
29946                
29947                
29948                
29949                
29951                
29952                
29953                
29954                
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
29956                
29957                
29958 08/21/13   Ramona No Yes Yes Yes  
29959                
29960 08/21/13   Ramona No Yes Yes Yes  
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
29966 08/22/13   Ramona No Yes Yes Yes  
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s
29972 08/22/13   Ramona No Yes Yes Yes  
29974                
29975     Ramona No Yes Yes Yes  
29976     Ramona No Yes Yes Yes  
29978                
29980     Ramona No Yes Yes Yes  
29981                
29982                
29983                
29984                
29985                
29986                
29987                
29988                
29989                
29991                
29992                
29993                
29994                
30024 09/04/13

30024_0.5_0.data

30024_0.5_1.data

30024_0.5_2.data

30024_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30025 09/04/13

30025_0.5_0.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes Bursts of 'overloads', periods of no data collection, were experienced. Very visibile between 200 and 300 ms.
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30029 09/04/13

30029_0.5_0.data

30029_0.5_1.data

30029_0.5_2.data

30029_0.5_3.data

 Omar Yes Yes Yes Yes After approximately .12 seconds the files consist mainly of noise.
30030 09/04/13

30030_0.5_0.data

30030_0.5_1.data

30030_0.5_2.data

30030_0.5_3.data

 Omar Yes Yes Yes Yes  
30031 09/04/13

30031_0.5_0.data

30031_0.5_1.data

30031_0.5_2.data

30031_0.5_3.data

 Omar Yes Yes Yes Yes  
30032 09/04/13

30032_0.5_0.data

30032_0.5_1.data

30032_0.5_2.data

30032_0.5_3.data

Omar Yes Yes Yes Yes  
30034 09/04/13

30034_0.5_0.data

30034_0.5_1.data

30034_0.5_2.data

30034_0.5_3.data

 Omar Yes Yes Yes Yes The peaks in channel 0 were difficult to distinguish due to periods of high noise and a base than had more noise than other shots at the base of the peak.
30035 09/04/13

30035_0.5_0.data

30035_0.5_1.data

30035_0.5_2.data

30035_0.5_3.data

 Omar Yes Yes Yes Yes  
30036 09/04/13

30036_0.5_0.data

30036_0.5_1.data

30036_0.5_2.data

30036_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30037 09/04/13

30037_0.5_0.data

30037_0.5_1.data

30037_0.5_2.data

30037_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30038 09/04/13

30038_0.5_0.data

30038_0.5_1.data

30038_0.5_2.data

30038_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30039 09/04/13

30039_0.5_0.data

30039_0.5_1.data

30039_0.5_2.data

30039_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.
30040 09/04/13

30040_0.5_0.data

30040_0.5_1.data

30040_0.5_2.data

30040_0.5_3.data

 Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.
30041 09/04/13

30041_0.5_0.data

30041_0.5_1.data

30041_0.5_2.data

30041_0.5_3.data

 Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.
30042 09/04/13

30042_0.5_0.data

30042_0.5_1.data

30042_0.5_2.data

30042_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.
30043 09/04/13

30043_0.5_0.data

30043_0.5_1.data

30043_0.5_2.data

30043_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .24 seconds.
30044 09/04/13

30044_0.5_0.data

30044_0.5_1.data

30044_0.5_2.data

30044_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .36 seconds.
30045                
30047                
30048                
30049                
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck
30051                
30052                
30053                
30054                
30055                
30056                
30057                
30058                
30059                
30060                
30062                
30063                
30064                
30065                
30066                
30067                
30068                
30069                
30071                
30073                
30074                
30075                
30076                
30077                
30078                
30079                
30080                
30081                
30082                
30084                
30085                
30086                
30087                
30088                
30089                
30090                
30091                
30092                
30093                
30094                
30095                
30097                
30098                
30099                
30100                
30101                
30102                
30103                
30104                
30105 09/09/13

30105_0.5_0.data

30105_0.5_1.data

30105_0.5_2.data

30105_0.5_3.data

 Pierre No No No No There are no particle peaks in any of the channels for this shot.
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre No No No No Ch 0 and Ch 1 have no particle peaks, but Ch 2 and Ch 3's signal are dominated by high frequency noise (Also no particle peaks).
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -2.7 V) at 0.163 sec amongst other smaller reflected peaks.
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec.

Ch 1 is a good signal.

Ch 2 is a good signal.

Ch 3 is a good signal.
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large noise peaks at 0.264 and 0.274 sec.

Ch 1 is a much cleaner signal than Ch 0.

Ch 2 is also a clean signal with little noise.

Ch 3 is also a clean signal with little noise.
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre Yes Yes Yes  

Ch 0 is very noisy with a few large high frequency waves of large amplitudes.

Ch 1 is considerably cleaner with only one large amplitude high frequency noise peak at 0.212 sec.

Ch 2 is also clean with a single large amplitude high frequency noise peak.

Ch 3 is a clean signal with a single large amplitude high frequency noise peak at 0.213 sec.
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre          
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre          
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre          
30125                
30126                
30127                
30128                
30130                
30131                
30132                
30133                
30134                
30135                
30136                
30137                
30138                
30139                
30140                
30141                
30142                
30143                
30144                
30145                
30147                
30148                
30149                
30150                
30151                
30152                
30153                
30154                
30155                
30156                
30157                
30158                
30159                
30160                
30162                
30163                
30164                
30165                
30166                
30167                
30168                
30169                
30170                
30171                
30172                
30173                
30174                
30175                
30176                
30177                
30178                
30179                
30180                
30181                
30182                
30183                
30184                
30185                
30187                
30188                
30189                
30190                
30191                
30192                
30193                
30194                
30195                
30196                
30197                
30198                
30199                
30200                
30201                
30202                
30203                
30204                
30205                
30206                
30207                
30208                
30209                
30210                
                 
>
>
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes  
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

   No Yes        
29807                  
29808                  
29809                  
29811                  
29812                  
29813                  
29814                  
29815                  
29818                  
29820                  
29821                  
29822                  
29823                  
29824                  
29825                  
29826                  
29827                  
29828                  
29829                  
29832                  
29834                  
29835                  
29837                  
29838                  
29839                  
29840                  
29841                  
29845                  
29846                  
29847                  
29848                  
29849                  
29851                  
29852                  
29853                  
29854                  
29855                  
29859                  
29862                  
29874                  
29875                  
29876                  
29877                  
29878                  
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes    
29880 08/19/13   Werner/ Ramona Yes No Yes Yes    
29881 08/19/13   Werner/ Ramona No Yes Yes Yes    
29882 08/19/13   Werner/ Ramona Yes No Yes Yes    
29883     Werner/ Ramona Yes Yes Yes Yes    
29884     Werner/ Ramona Yes Yes Yes Yes    
29885     Werner/ Ramona Yes Yes Yes Yes    
29890                  
29891                  
29892                  
29893                  
29894                  
29895                  
29896                  
29897                  
29898                  
29899 08/20/13   Douglas No No No No All channels only noise.  
29901 08/20/13   Douglas No No No No All channels only noise.  
29902 08/20/13   Douglas No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.  
29904 08/20/13   Pierre/ Ramona No No No No    
29905 08/20/13   Pierre/ Ramona No No No No    
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Omar/ Ramona

Douglas

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise

  
29907 08/20/13

29907_0.5_0.data

29907_0.5_1.data

29907_0.5_2.data

29907_0.5_3.data

 Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)  
29908 08/20/13

29908_0.5_0.data

29908_0.5_2.data

29908_0.5_3.data

Pierre

Douglas

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.

  
29909 08/20/13

29909_0.5_0.data

29909_0.5_1.data

29909_0.5_2.data

29909_0.5_3.data

 Ramona/ Pierre Yes Yes Yes Yes    
29910 08/20/13

29910_0.5_1.data

29910_0.5_2.data

29910_0.5_3.data

 Ramona/ Pierre No Yes Yes Yes    
29911 08/20/13   Douglas No No No No    
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

 Douglas No Yes Yes Yes    
29914 08/20/13

29914_0.5_1.data

29914_0.5_2.data

29914_0.5_3.data

 Douglas No Yes Yes Yes    
29915 08/20/13

29915_0.5_1.data

29915_0.5_2.data

29915_0.5_3.data

 Douglas No Yes Yes Yes    
29916 08/20/13   Douglas No No No No    
29917 08/20/13

29917_0.5_1.data

29917_0.5_2.data

29917_0.5_3.data

 Ramona No Yes Yes Yes    
29918 08/20/13   Douglas No No No No    
29919 08/2013

29919_0.5_1.data

29919_0.5_2.data

29919_0.5_3.data

Douglas

 No Yes Yes Yes    
29920 08/20/13

29920_0.5_1.data

29920_0.5_2.data

29920_0.5_3.data

Werner

Douglas

 No Yes Yes Yes    
29921 08/20/13

29921_0.5_2.data

29921_0.5_3.data

 Douglas No No Yes Yes    
29922 08/20/13

29922_0.5_1.data

29922_0.5_2.data

29922_0.5_3.data

 Douglas No Yes Yes Yes    
29923 08/20/13

29923_0.5_1.data

29923_0.5_2.data

29923_0.5_3.data

 Douglas No Yes Yes Yes    
29924 08/20/13

29924_0.5_0.data

29924_0.5_1.data

29924_0.5_2.data

29924_0.5_3.data

Ramona/ Omar

Douglas

 No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.  
29925 08/20/13

29925_0.5_1.data

29925_0.5_2.data

29925_0.5_3.data

 Douglas No Yes Yes Yes    
29926 08/20/13   Douglas No No No No    
29927 08/20/13   Douglas No No No No    
29928 08/20/13   Ramona No Yes Yes Yes    
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.  
29930 08/20/13   Douglas No No No No All channels mostly noise.  
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes    
29932                  
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise  
29934                  
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes    
29936                  
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes    
29938                  
29939                  
29940                  
29941                  
29942                  
29943                  
29944                  
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3

  
29946                  
29947                  
29948                  
29949                  
29951                  
29952                  
29953                  
29954                  
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts  
29956                  
29957                  
29958 08/21/13   Ramona No Yes Yes Yes    
29959                  
29960 08/21/13   Ramona No Yes Yes Yes    
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s  
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise  
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise  
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s

  
29966 08/22/13   Ramona No Yes Yes Yes    
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise

  
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s

  
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s  
29972 08/22/13   Ramona No Yes Yes Yes    
29974                  
29975     Ramona No Yes Yes Yes    
29976     Ramona No Yes Yes Yes    
29978                  
29980     Ramona No Yes Yes Yes    
29981                  
29982                  
29983                  
29984                  
29985                  
29986                  
29987                  
29988                  
29989                  
29991                  
29992                  
29993                  
29994                  
30024 09/04/13

30024_0.5_0.data

30024_0.5_1.data

30024_0.5_2.data

30024_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.  
30025 09/04/13

30025_0.5_0.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.  
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes Bursts of 'overloads', periods of no data collection, were experienced. Very visibile between 200 and 300 ms.  
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.  
30029 09/04/13

30029_0.5_0.data

30029_0.5_1.data

30029_0.5_2.data

30029_0.5_3.data

 Omar Yes Yes Yes Yes After approximately .12 seconds the files consist mainly of noise.  
30030 09/04/13

30030_0.5_0.data

30030_0.5_1.data

30030_0.5_2.data

30030_0.5_3.data

 Omar Yes Yes Yes Yes    
30031 09/04/13

30031_0.5_0.data

30031_0.5_1.data

30031_0.5_2.data

30031_0.5_3.data

 Omar Yes Yes Yes Yes    
30032 09/04/13

30032_0.5_0.data

30032_0.5_1.data

30032_0.5_2.data

30032_0.5_3.data

Omar Yes Yes Yes Yes    
30034 09/04/13

30034_0.5_0.data

30034_0.5_1.data

30034_0.5_2.data

30034_0.5_3.data

 Omar Yes Yes Yes Yes The peaks in channel 0 were difficult to distinguish due to periods of high noise and a base than had more noise than other shots at the base of the peak.  
30035 09/04/13

30035_0.5_0.data

30035_0.5_1.data

30035_0.5_2.data

30035_0.5_3.data

 Omar Yes Yes Yes Yes    
30036 09/04/13

30036_0.5_0.data

30036_0.5_1.data

30036_0.5_2.data

30036_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.  
30037 09/04/13

30037_0.5_0.data

30037_0.5_1.data

30037_0.5_2.data

30037_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.  
30038 09/04/13

30038_0.5_0.data

30038_0.5_1.data

30038_0.5_2.data

30038_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.  
30039 09/04/13

30039_0.5_0.data

30039_0.5_1.data

30039_0.5_2.data

30039_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.  
30040 09/04/13

30040_0.5_0.data

30040_0.5_1.data

30040_0.5_2.data

30040_0.5_3.data

 Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.  
30041 09/04/13

30041_0.5_0.data

30041_0.5_1.data

30041_0.5_2.data

30041_0.5_3.data

 Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.  
30042 09/04/13

30042_0.5_0.data

30042_0.5_1.data

30042_0.5_2.data

30042_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.  
30043 09/04/13

30043_0.5_0.data

30043_0.5_1.data

30043_0.5_2.data

30043_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .24 seconds.  
30044 09/04/13

30044_0.5_0.data

30044_0.5_1.data

30044_0.5_2.data

30044_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .36 seconds.  
30045                  
30047                  
30048                  
30049                  
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck

  
30051                  
30052                  
30053                  
30054                  
30055                  
30056                  
30057                  
30058                  
30059                  
30060                  
30062                  
30063                  
30064                  
30065                  
30066                  
30067                  
30068                  
30069                  
30071                  
30073                  
30074                  
30075                  
30076                  
30077                  
30078                  
30079                  
30080                  
30081                  
30082                  
30084                  
30085                  
30086                  
30087                  
30088                  
30089                  
30090                  
30091                  
30092                  
30093                  
30094                  
30095                  
30097                  
30098                  
30099                  
30100                  
30101                  
30102                  
30103                  
30104                  
30105 09/09/13

30105_0.5_0.data

30105_0.5_1.data

30105_0.5_2.data

30105_0.5_3.data

 Pierre No No No No There are no particle peaks in any of the channels for this shot.  
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre No No No No Ch 0 and Ch 1 have no particle peaks, but Ch 2 and Ch 3's signal are dominated by high frequency noise (Also no particle peaks).  
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

  
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -2.7 V) at 0.163 sec amongst other smaller reflected peaks.

  
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes    
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes    
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise

  
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms

  
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.

  
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.  
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

  
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec.

Ch 1 is a good signal.

Ch 2 is a good signal.

Ch 3 is a good signal.

  
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large noise peaks at 0.264 and 0.274 sec.

Ch 1 is a much cleaner signal than Ch 0.

Ch 2 is also a clean signal with little noise.

Ch 3 is also a clean signal with little noise.

  
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.  
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.

  
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.

  
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre No Yes Yes Yes

Ch 0 is very noisy with a few large high frequency waves of large amplitudes.

Ch 1 is considerably cleaner with only one large amplitude high frequency noise peak at 0.212 sec.

Ch 2 is also clean with a single large amplitude high frequency noise peak.

Ch 3 is a clean signal with a single large amplitude high frequency noise peak at 0.213 sec.

  
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has quite a few reflected peaks and a large noise peak at 0.211 sec. There is a lot of low voltage noise embedded in the baseline signal.

Ch 1 is a cleaner signal than Ch 0 with a few reflected noise peaks.

Ch 2 is a cleaner signal than Ch 0 but with a noiser baseline signal.

Ch 3 is a cleaner signal than Ch 0 but with a noiser baseline signal.

  
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre            
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre            
30125                  
30126                  
30127                  
30128                  
30130                  
30131                  
30132                  
30133                  
30134                  
30135                  
30136                  
30137                  
30138                  
30139                  
30140                  
30141                  
30142                  
30143                  
30144                  
30145                  
30147                  
30148                  
30149                  
30150                  
30151                  
30152                  
30153                  
30154                  
30155                  
30156                  
30157                  
30158                  
30159                  
30160                  
30162                  
30163                  
30164                  
30165                  
30166                  
30167                  
30168                  
30169                  
30170                  
30171                  
30172                  
30173                  
30174                  
30175                  
30176                  
30177                  
30178                  
30179                  
30180                  
30181                  
30182                  
30183                  
30184                  
30185                  
30187                  
30188                  
30189                  
30190                  
30191                  
30192                  
30193                  
30194                  
30195                  
30196                  
30197                  
30198                  
30199                  
30200                  
30201                  
30202                  
30203                  
30204                  
30205                  
30206                  
30207                  
30208                  
30209                  
30210                  
                   
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 662014-06-09 - Dtuck001

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 118 to 118
 
29898                
29899 08/20/13   Douglas No No No No All channels only noise.
29901 08/20/13   Douglas No No No No All channels only noise.
Changed:
<
<
29902 08/20/13   Dougla No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.
>
>
29902 08/20/13   Douglas No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.
 
29904 08/20/13   Pierre/ Ramona No No No No  
29905 08/20/13   Pierre/ Ramona No No No No  
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Omar/ Ramona

Douglas

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise
Changed:
<
<
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
>
>
29907 08/20/13

29907_0.5_0.data

29907_0.5_1.data

29907_0.5_2.data

29907_0.5_3.data

 Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
 
29908 08/20/13

29908_0.5_0.data

29908_0.5_2.data

29908_0.5_3.data

Pierre

Douglas

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.
Changed:
<
<
29909 08/20/13   Ramona/ Pierre Yes Yes Yes Yes  
29910 08/20/13   Ramona/ Pierre No Yes Yes Yes  
>
>
29909 08/20/13

29909_0.5_0.data

29909_0.5_1.data

29909_0.5_2.data

29909_0.5_3.data

 Ramona/ Pierre Yes Yes Yes Yes  
29910 08/20/13

29910_0.5_1.data

29910_0.5_2.data

29910_0.5_3.data

 Ramona/ Pierre No Yes Yes Yes  
 
29911 08/20/13   Douglas No No No No  
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

 Douglas No Yes Yes Yes  
29914 08/20/13

29914_0.5_1.data

29914_0.5_2.data

29914_0.5_3.data

 Douglas No Yes Yes Yes  
29915 08/20/13

29915_0.5_1.data

29915_0.5_2.data

29915_0.5_3.data

 Douglas No Yes Yes Yes  
29916 08/20/13   Douglas No No No No  
Changed:
<
<
29917 08/20/13   Ramona No Yes Yes Yes  
29918 08/20/13     No No No No  
29919 08/2013 29915_0.5_1.data Douglas No Yes Yes Yes  
29920 08/20/13   Werner          
29921                
29922                
29923                
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925                
29926                
29927                
29928     Ramona No Yes Yes Yes  
>
>
29917 08/20/13

29917_0.5_1.data

29917_0.5_2.data

29917_0.5_3.data

 Ramona No Yes Yes Yes  
29918 08/20/13   Douglas No No No No  
29919 08/2013

29919_0.5_1.data

29919_0.5_2.data

29919_0.5_3.data

Douglas

 No Yes Yes Yes  
29920 08/20/13

29920_0.5_1.data

29920_0.5_2.data

29920_0.5_3.data

Werner

Douglas

 No Yes Yes Yes  
29921 08/20/13

29921_0.5_2.data

29921_0.5_3.data

 Douglas No No Yes Yes  
29922 08/20/13

29922_0.5_1.data

29922_0.5_2.data

29922_0.5_3.data

 Douglas No Yes Yes Yes  
29923 08/20/13

29923_0.5_1.data

29923_0.5_2.data

29923_0.5_3.data

 Douglas No Yes Yes Yes  
29924 08/20/13

29924_0.5_0.data

29924_0.5_1.data

29924_0.5_2.data

29924_0.5_3.data

Ramona/ Omar

Douglas

 No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925 08/20/13

29925_0.5_1.data

29925_0.5_2.data

29925_0.5_3.data

 Douglas No Yes Yes Yes  
29926 08/20/13   Douglas No No No No  
29927 08/20/13   Douglas No No No No  
29928 08/20/13   Ramona No Yes Yes Yes  
 
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
Changed:
<
<
29930                
>
>
29930 08/20/13   Douglas No No No No All channels mostly noise.
 
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
29932                
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise

Revision 652014-06-07 - Dtuck001

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 121 to 121
 
29902 08/20/13   Dougla No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.
29904 08/20/13   Pierre/ Ramona No No No No  
29905 08/20/13   Pierre/ Ramona No No No No  
Changed:
<
<
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
>
>
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

29906_0.5_2.data

29906_0.5_3.data

Omar/ Ramona

Douglas

 Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Ch2, Ch3: Good from 0.1s to 0.3 s. After that only noise
 
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
Changed:
<
<
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
>
>
29908 08/20/13

29908_0.5_0.data

29908_0.5_2.data

29908_0.5_3.data

Pierre

Douglas

 No No Yes Yes

Ch0: This channel does not exhibit any charged particle peaks

Ch1: Possible overload from 0.1s to 0.3s. No charged particles peaks present.

Ch2, Ch3: Good from 0.1s to 0.3s.
 
29909 08/20/13   Ramona/ Pierre Yes Yes Yes Yes  
29910 08/20/13   Ramona/ Pierre No Yes Yes Yes  
29911 08/20/13   Douglas No No No No  

Revision 642014-06-06 - omaleo21

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 215 to 215
 
30037 09/04/13

30037_0.5_0.data

30037_0.5_1.data

30037_0.5_2.data

30037_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30038 09/04/13

30038_0.5_0.data

30038_0.5_1.data

30038_0.5_2.data

30038_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30039 09/04/13

30039_0.5_0.data

30039_0.5_1.data

30039_0.5_2.data

30039_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.
Changed:
<
<
30040                
30041                
30042                
30043                
30044                
>
>
30040 09/04/13

30040_0.5_0.data

30040_0.5_1.data

30040_0.5_2.data

30040_0.5_3.data

Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.
30041 09/04/13

30041_0.5_0.data

30041_0.5_1.data

30041_0.5_2.data

30041_0.5_3.data

Omar No Yes Yes Yes Channel 0 may be composed entirely of noise.
30042 09/04/13

30042_0.5_0.data

30042_0.5_1.data

30042_0.5_2.data

30042_0.5_3.data

Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.
30043 09/04/13

30043_0.5_0.data

30043_0.5_1.data

30043_0.5_2.data

30043_0.5_3.data

Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .24 seconds.
30044 09/04/13

30044_0.5_0.data

30044_0.5_1.data

30044_0.5_2.data

30044_0.5_3.data

Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks. There is no apparent data after approximately .36 seconds.
 
30045                
30047                
30048                

Revision 632014-06-04 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 290 to 290
 
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.
Changed:
<
<
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre Yes       Ch 0 is very noisy with a few large high frequency waves of large amplitudes.
>
>
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre Yes Yes Yes  

Ch 0 is very noisy with a few large high frequency waves of large amplitudes.

Ch 1 is considerably cleaner with only one large amplitude high frequency noise peak at 0.212 sec.

Ch 2 is also clean with a single large amplitude high frequency noise peak.

Ch 3 is a clean signal with a single large amplitude high frequency noise peak at 0.213 sec.
 
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre          
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre          
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre          

Revision 622014-06-04 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 290 to 290
 
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.
Changed:
<
<
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre          
>
>
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre Yes       Ch 0 is very noisy with a few large high frequency waves of large amplitudes.
 
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre          
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre          
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre          

Revision 612014-06-03 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Revision 602014-06-02 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 290 to 290
 
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.
Changed:
<
<
30121                
30122                
30123                
30124                
>
>
30121 09/09/13

30121_0.5_0.data

30121_0.5_1.data

30121_0.5_2.data

30121_0.5_3.data

 Pierre          
30122 09/09/13

30122_0.5_0.data

30122_0.5_1.data

30122_0.5_2.data

30122_0.5_3.data

 Pierre          
30123 09/09/13

30123_0.5_0.data

30123_0.5_1.data

30123_0.5_2.data

30123_0.5_3.data

 Pierre          
30124 09/09/13

30124_0.5_0.data

30124_0.5_1.data

30124_0.5_2.data

30124_0.5_3.data

 Pierre          
 
30125                
30126                
30127                

Revision 592014-05-30 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 287 to 287
 
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec.

Ch 1 is a good signal.

Ch 2 is a good signal.

Ch 3 is a good signal.
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large noise peaks at 0.264 and 0.274 sec.

Ch 1 is a much cleaner signal than Ch 0.

Ch 2 is also a clean signal with little noise.

Ch 3 is also a clean signal with little noise.
Changed:
<
<
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre          
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre          
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre          
>
>
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre No No No No Ch 2 is all high frequency high voltage noise.
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre No No No No

Ch 2 is all high frequency high voltage noise.

Ch 3 is all high frequency high voltage noise.
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0's signal ends after 0.132 sec.

Ch 1's signal ends after 0.136 sec. Peaks are cleaner than in Ch 0.

Ch 2's signal ends after 0.135 sec. There is much more noise prevelant in the signal.

Ch 3's signal ends after 0.145 sec. There is much more noise prevelant in the signal but not as high in amplitude.
 
30121                
30122                
30123                

Revision 582014-05-30 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 286 to 286
 
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec.

Ch 1 is a good signal.

Ch 2 is a good signal.

Ch 3 is a good signal.
Changed:
<
<
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre          
>
>
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has two large noise peaks at 0.264 and 0.274 sec.

Ch 1 is a much cleaner signal than Ch 0.

Ch 2 is also a clean signal with little noise.

Ch 3 is also a clean signal with little noise.
 
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre          
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre          
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre          

Revision 572014-05-30 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 224 to 224
 
30047                
30048                
30049                
Changed:
<
<
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks CARLOS WE NEVER TOOK DATA May 5th

Ch1: Noisier than Ch0, found no real peaks, will recheck
>
>
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck
 
30051                
30052                
30053                

Revision 562014-05-30 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 53 to 53
 
091113
091213
Added:
>
>		Yes
 
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

   No Yes      
29807                
Line: 209 to 210
 
30031 09/04/13

30031_0.5_0.data

30031_0.5_1.data

30031_0.5_2.data

30031_0.5_3.data

 Omar Yes Yes Yes Yes  
30032 09/04/13

30032_0.5_0.data

30032_0.5_1.data

30032_0.5_2.data

30032_0.5_3.data

Omar Yes Yes Yes Yes  
30034 09/04/13

30034_0.5_0.data

30034_0.5_1.data

30034_0.5_2.data

30034_0.5_3.data

 Omar Yes Yes Yes Yes The peaks in channel 0 were difficult to distinguish due to periods of high noise and a base than had more noise than other shots at the base of the peak.
Changed:
<
<
30035                
30036                
30037                
30038                
30039                
>
>
30035 09/04/13

30035_0.5_0.data

30035_0.5_1.data

30035_0.5_2.data

30035_0.5_3.data

 Omar Yes Yes Yes Yes  
30036 09/04/13

30036_0.5_0.data

30036_0.5_1.data

30036_0.5_2.data

30036_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30037 09/04/13

30037_0.5_0.data

30037_0.5_1.data

30037_0.5_2.data

30037_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30038 09/04/13

30038_0.5_0.data

30038_0.5_1.data

30038_0.5_2.data

30038_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection.
30039 09/04/13

30039_0.5_0.data

30039_0.5_1.data

30039_0.5_2.data

30039_0.5_3.data

 Omar No Yes Yes Yes Channel 0 has noisy peaks which make it difficult to provide a consistent selection. Whole channel may be all noise with very few peaks.
 
30040                
30041                
30042                
Line: 223 to 224
 
30047                
30048                
30049                
Changed:
<
<
30050 05/09/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks CARLOS WE NEVER TOOK DATA May 5th

Ch1: Noisier than Ch0, found no real peaks, will recheck
>
>
30050 09/05/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks CARLOS WE NEVER TOOK DATA May 5th

Ch1: Noisier than Ch0, found no real peaks, will recheck
 
30051                
30052                
30053                

Revision 552014-05-29 - Dtuck001

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 115 to 115
 
29896                
29897                
29898                
Changed:
<
<
29899                
29901                
29902                
29904     Pierre/ Ramona No No No No  
29905     Pierre/ Ramona No No No No  
>
>
29899 08/20/13   Douglas No No No No All channels only noise.
29901 08/20/13   Douglas No No No No All channels only noise.
29902 08/20/13   Dougla No No No No Ch.0,2,3 - Quiescent; Ch.1 only noise.
29904 08/20/13   Pierre/ Ramona No No No No  
29905 08/20/13   Pierre/ Ramona No No No No  
 
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
Changed:
<
<
29909     Ramona/ Pierre Yes Yes Yes Yes  
29910     Ramona/ Pierre No Yes Yes Yes  
>
>
29909 08/20/13   Ramona/ Pierre Yes Yes Yes Yes  
29910 08/20/13   Ramona/ Pierre No Yes Yes Yes  
 
29911 08/20/13   Douglas No No No No  
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

 Douglas No Yes Yes Yes  
Changed:
<
<
29914                
29915                
29916                
29917     Ramona No Yes Yes Yes  
29918                
29919                
>
>
29914 08/20/13

29914_0.5_1.data

29914_0.5_2.data

29914_0.5_3.data

 Douglas No Yes Yes Yes  
29915 08/20/13

29915_0.5_1.data

29915_0.5_2.data

29915_0.5_3.data

 Douglas No Yes Yes Yes  
29916 08/20/13   Douglas No No No No  
29917 08/20/13   Ramona No Yes Yes Yes  
29918 08/20/13     No No No No  
29919 08/2013 29915_0.5_1.data Douglas No Yes Yes Yes  
 
29920 08/20/13   Werner          
29921                
29922                

Revision 542014-05-27 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 284 to 284
 
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
Changed:
<
<
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes       Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec
>
>
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec.

Ch 1 is a good signal.

Ch 2 is a good signal.

Ch 3 is a good signal.
 
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre          
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre          
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre          

Revision 532014-05-27 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 284 to 284
 
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
Changed:
<
<
30116                
30117                
30118                
30119                
30120                
>
>
30116 09/09/13

30116_0.5_0.data

30116_0.5_1.data

30116_0.5_2.data

30116_0.5_3.data

 Pierre Yes       Ch 0 has small reflected peaks [0.084, 0.152] and at 0.291 and 0.307 sec
30117 09/09/13

30117_0.5_0.data

30117_0.5_1.data

30117_0.5_2.data

30117_0.5_3.data

 Pierre          
30118 09/09/13

30118_0.5_0.data

30118_0.5_1.data

30118_0.5_2.data

30118_0.5_3.data

 Pierre          
30119 09/09/13

30119_0.5_0.data

30119_0.5_1.data

30119_0.5_2.data

30119_0.5_3.data

 Pierre          
30120 09/09/13

30120_0.5_0.data

30120_0.5_1.data

30120_0.5_2.data

30120_0.5_3.data

 Pierre          
 
30121                
30122                
30123                

Revision 522014-05-27 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 283 to 283
 
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
Changed:
<
<
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes        
>
>
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has many large amplitude (~3 V) high frequency reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 1 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 2 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]

Ch 3 has a few moderate amplitude (~ 2 V) reflected peaks. Look for outliers in rates [0.126, 0.250]
 
30116                
30117                
30118                

Revision 512014-05-26 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 283 to 283
 
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
Changed:
<
<
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre          
>
>
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre Yes        
 
30116                
30117                
30118                

Revision 502014-05-24 - Dtuck001

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 125 to 125
 
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909     Ramona/ Pierre Yes Yes Yes Yes  
29910     Ramona/ Pierre No Yes Yes Yes  
Changed:
<
<
29911                
29912                
>
>
29911 08/20/13   Douglas No No No No  
29912 08/20/13

29912_0.5_1.data

29912_0.5_2.data

29912_0.5_3.data

Douglas No Yes Yes Yes  
 
29914                
29915                
29916                

Revision 492014-05-22 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 276 to 276
 
30105 09/09/13

30105_0.5_0.data

30105_0.5_1.data

30105_0.5_2.data

30105_0.5_3.data

 Pierre No No No No There are no particle peaks in any of the channels for this shot.
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre No No No No Ch 0 and Ch 1 have no particle peaks, but Ch 2 and Ch 3's signal are dominated by high frequency noise (Also no particle peaks).
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec
Changed:
<
<
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes  
>
>
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has a large reflected peak (~ -2.7 V) at 0.163 sec amongst other smaller reflected peaks.
 
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
Changed:
<
<
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre          
>
>
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre Yes Yes Yes Yes Ch 0, Ch 1, Ch 2, Ch 3 has some reflected peaks but nothing too large.
 
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre          
30116                
30117                

Revision 482014-05-21 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 280 to 280
 
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise
Changed:
<
<
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes    

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre          
>
>
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0 has high frequency and high voltage noise [0.166, 0.198]

Ch 1 has two large reflected peaks at 0.167 sec and 0.190 sec.

Ch 2 has a high voltage (~3.5 V) and high frequency noise spike at 0.189 sec.

Ch 3 has large reflected (~ -1 V) peaks at 0.167, 0.170, and 0.189 sec.
 
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre          
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre          
30116                

Revision 472014-05-21 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 204 to 204
 
30025 09/04/13

30025_0.5_0.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes Bursts of 'overloads', periods of no data collection, were experienced. Very visibile between 200 and 300 ms.
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
Changed:
<
<
30029                
30030                
30031                
30032                
30034                
>
>
30029 09/04/13

30029_0.5_0.data

30029_0.5_1.data

30029_0.5_2.data

30029_0.5_3.data

 Omar Yes Yes Yes Yes After approximately .12 seconds the files consist mainly of noise.
30030 09/04/13

30030_0.5_0.data

30030_0.5_1.data

30030_0.5_2.data

30030_0.5_3.data

 Omar Yes Yes Yes Yes  
30031 09/04/13

30031_0.5_0.data

30031_0.5_1.data

30031_0.5_2.data

30031_0.5_3.data

Omar Yes Yes Yes Yes  
30032 09/04/13

30032_0.5_0.data

30032_0.5_1.data

30032_0.5_2.data

30032_0.5_3.data

Omar Yes Yes Yes Yes  
30034 09/04/13

30034_0.5_0.data

30034_0.5_1.data

30034_0.5_2.data

30034_0.5_3.data

Omar Yes Yes Yes Yes The peaks in channel 0 were difficult to distinguish due to periods of high noise and a base than had more noise than other shots at the base of the peak.
 
30035                
30036                
30037                

Revision 462014-05-20 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 280 to 280
 
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise
Changed:
<
<
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre          
>
>
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre Yes Yes    

Ch 1 has a large peak (~3.5 V) at 288 ms

Ch 2 has a large peak (~3.5 V) at 289 ms
 
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre          
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre          
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre          

Revision 452014-05-19 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

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30047                
30048                
30049                
Changed:
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30050 05/09/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck
>
>
30050 05/09/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks CARLOS WE NEVER TOOK DATA May 5th

Ch1: Noisier than Ch0, found no real peaks, will recheck
 
30051                
30052                
30053                
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30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes  
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
Changed:
<
<
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes        
30112                
30113                
30114                
30115                
>
>
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes Yes Yes Yes

Ch 0, there are some high frequency high voltage around 100 ms into the shot

Ch 1, the signal seems to being prematurely and there is some high frequency noise

Ch 2, the signal seems to being prematurely and there is some high frequency noise

Ch 3, the signal seems to being prematurely and there is some high frequency noise
30112 09/09/13

30112_0.5_0.data

30112_0.5_1.data

30112_0.5_2.data

30112_0.5_3.data

 Pierre          
30113 09/09/13

30113_0.5_0.data

30113_0.5_1.data

30113_0.5_2.data

30113_0.5_3.data

 Pierre          
30114 09/09/13

30114_0.5_0.data

30114_0.5_1.data

30114_0.5_2.data

30114_0.5_3.data

 Pierre          
30115 09/09/13

30115_0.5_0.data

30115_0.5_1.data

30115_0.5_2.data

30115_0.5_3.data

 Pierre          
 
30116                
30117                
30118                

Revision 442014-05-19 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 278 to 278
 
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes  
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre Yes Yes Yes Yes  
Changed:
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<
30110 09/09/13

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 Pierre          
30111                
>
>
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre Yes Yes Yes Yes  
30111 09/09/13

30111_0.5_0.data

30111_0.5_1.data

30111_0.5_2.data

30111_0.5_3.data

 Pierre Yes        
 
30112                
30113                
30114                

Revision 432014-05-19 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 277 to 277
 
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre No No No No Ch 0 and Ch 1 have no particle peaks, but Ch 2 and Ch 3's signal are dominated by high frequency noise (Also no particle peaks).
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes  
Changed:
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<
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>
>
30109 09/09/13

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30109_0.5_2.data

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 Pierre Yes Yes Yes Yes  
 
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre          
30111                
30112                

Revision 422014-05-17 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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30102                
30103                
30104                
Changed:
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30105 09/09/13

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30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre          
30107 09/09/13

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30107_0.5_3.data

 Pierre          
30108 09/09/13

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 Pierre          
30109  

30109_0.5_0.data

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 Pierre          
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 Pierre          
>
>
30105 09/09/13

30105_0.5_0.data

30105_0.5_1.data

30105_0.5_2.data

30105_0.5_3.data

 Pierre No No No No There are no particle peaks in any of the channels for this shot.
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre No No No No Ch 0 and Ch 1 have no particle peaks, but Ch 2 and Ch 3's signal are dominated by high frequency noise (Also no particle peaks).
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre No No No No

Ch 0 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 1 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 2 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec

Ch 3 has a singular high frequency high voltage (~3 V) noise peak @ 0.452 sec
30108 09/09/13

30108_0.5_0.data

30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre Yes Yes Yes Yes  
30109 09/09/13

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre          
30110 09/09/13

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre          
 
30111                
30112                
30113                

Revision 412014-05-17 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 54 to 54
 
091213

Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
Changed:
<
<
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes      
>
>
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

   No Yes      
 
29807                
29808                
29809                
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30102                
30103                
30104                
Changed:
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30105                
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30110                
>
>
30105 09/09/13

30105_0.5_0.data

30105_0.5_1.data

30105_0.5_2.data

30105_0.5_3.data

 Pierre          
30106 09/09/13

30106_0.5_0.data

30106_0.5_1.data

30106_0.5_2.data

30106_0.5_3.data

 Pierre          
30107 09/09/13

30107_0.5_0.data

30107_0.5_1.data

30107_0.5_2.data

30107_0.5_3.data

 Pierre          
30108 09/09/13

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30108_0.5_1.data

30108_0.5_2.data

30108_0.5_3.data

 Pierre          
30109  

30109_0.5_0.data

30109_0.5_1.data

30109_0.5_2.data

30109_0.5_3.data

 Pierre          
30110  

30110_0.5_0.data

30110_0.5_1.data

30110_0.5_2.data

30110_0.5_3.data

 Pierre          
 
30111                
30112                
30113                

Revision 402014-05-16 - clope023

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 223 to 223
 
30047                
30048                
30049                
Changed:
<
<
30050                
>
>
30050 05/09/2013

30050_0.5_0.data

30050_0.5_1.data

30050_0.5_2.data

30050_0.5_3.data

 Carlos Yes No Yes Yes

Ch0: Very noisy, but found 3 peaks

Ch1: Noisier than Ch0, found no real peaks, will recheck
 
30051                
30052                
30053                

Revision 392014-05-16 - omaleo21

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 53 to 53
 
091113
091213
Changed:
<
<
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes
29807
29808
29809
29811
29812
29813
29814
29815
29818
29820
29821
29822
29823
29824
29825
29826
29827
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29829
29832
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29841
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29846
29847
29848
29849
29851
29852
29853
29854
29855
29859
29862
29874
29875
29876
29877
29878
29879 08/19/13 Werner/ Ramona Yes Yes Yes Yes
29880 08/19/13 Werner/ Ramona Yes No Yes Yes
29881 08/19/13 Werner/ Ramona No Yes Yes Yes
29882 08/19/13 Werner/ Ramona Yes No Yes Yes
29883 Werner/ Ramona Yes Yes Yes Yes
29884 Werner/ Ramona Yes Yes Yes Yes
29885 Werner/ Ramona Yes Yes Yes Yes
29890
29891
29892
29893
29894
29895
29896
29897
29898
29899
29901
29902
29904 Pierre/ Ramona No No No No
29905 Pierre/ Ramona No No No No
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No Ch0: This channel does not exhibit any charged particle peaks
29909 Ramona/ Pierre Yes Yes Yes Yes
29910 Ramona/ Pierre No Yes Yes Yes
29911
29912
29914
29915
29916
29917 Ramona No Yes Yes Yes
29918
29919
29920 08/20/13 Werner
29921
29922
29923
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925
29926
29927
29928 Ramona No Yes Yes Yes
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
29930
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes
29932
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
29934
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes
29936
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes
29938
29939
29940
29941
29942
29943
29944
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
29946
29947
29948
29949
29951
29952
29953
29954
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
29956
29957
29958 08/21/13 Ramona No Yes Yes Yes
29959
29960 08/21/13 Ramona No Yes Yes Yes
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
29966 08/22/13 Ramona No Yes Yes Yes
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes Ch1: There is only noise after t = .286s
29972 08/22/13 Ramona No Yes Yes Yes
29974
29975 Ramona No Yes Yes Yes
29976// Ramona No Yes Yes Yes
29978
29980 Ramona No Yes Yes Yes
29981
29982
29983
29984
29985
29986
29987
29988
29989
29991
29992
29993
29994
30024 09/04/13

30024_0.5_0.data

30024_0.5_1.data

30024_0.5_2.data

30024_0.5_3.data

 Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
30025 09/04/13

30025_0.5_1.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes All channels had short burts of "overloads" (No registered data). These are very apparent between 200 and 300 ms.
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
>
>
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes      
29807                
29808                
29809                
29811                
29812                
29813                
29814                
29815                
29818                
29820                
29821                
29822                
29823                
29824                
29825                
29826                
29827                
29828                
29829                
29832                
29834                
29835                
29837                
29838                
29839                
29840                
29841                
29845                
29846                
29847                
29848                
29849                
29851                
29852                
29853                
29854                
29855                
29859                
29862                
29874                
29875                
29876                
29877                
29878                
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes  
29880 08/19/13   Werner/ Ramona Yes No Yes Yes  
29881 08/19/13   Werner/ Ramona No Yes Yes Yes  
29882 08/19/13   Werner/ Ramona Yes No Yes Yes  
29883     Werner/ Ramona Yes Yes Yes Yes  
29884     Werner/ Ramona Yes Yes Yes Yes  
29885     Werner/ Ramona Yes Yes Yes Yes  
29890                
29891                
29892                
29893                
29894                
29895                
29896                
29897                
29898                
29899                
29901                
29902                
29904     Pierre/ Ramona No No No No  
29905     Pierre/ Ramona No No No No  
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909     Ramona/ Pierre Yes Yes Yes Yes  
29910     Ramona/ Pierre No Yes Yes Yes  
29911                
29912                
29914                
29915                
29916                
29917     Ramona No Yes Yes Yes  
29918                
29919                
29920 08/20/13   Werner          
29921                
29922                
29923                
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925                
29926                
29927                
29928     Ramona No Yes Yes Yes  
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
29930                
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
29932                
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
29934                
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes  
29936                
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes  
29938                
29939                
29940                
29941                
29942                
29943                
29944                
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
29946                
29947                
29948                
29949                
29951                
29952                
29953                
29954                
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
29956                
29957                
29958 08/21/13   Ramona No Yes Yes Yes  
29959                
29960 08/21/13   Ramona No Yes Yes Yes  
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
29966 08/22/13   Ramona No Yes Yes Yes  
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s
29972 08/22/13   Ramona No Yes Yes Yes  
29974                
29975     Ramona No Yes Yes Yes  
29976     Ramona No Yes Yes Yes  
29978                
29980     Ramona No Yes Yes Yes  
29981                
29982                
29983                
29984                
29985                
29986                
29987                
29988                
29989                
29991                
29992                
29993                
29994                
30024 09/04/13

30024_0.5_0.data

30024_0.5_1.data

30024_0.5_2.data

30024_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30025 09/04/13

30025_0.5_0.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes Bursts of 'overloads', periods of no data collection, were experienced. Very visibile between 200 and 300 ms.
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or were too noisy for data analysis.
30029                
30030                
30031                
30032                
30034                
30035                
30036                
30037                
30038                
30039                
30040                
30041                
30042                
30043                
30044                
30045                
30047                
30048                
30049                
30050                
30051                
30052                
30053                
30054                
30055                
30056                
30057                
30058                
30059                
30060                
30062                
30063                
30064                
30065                
30066                
30067                
30068                
30069                
30071                
30073                
30074                
30075                
30076                
30077                
30078                
30079                
30080                
30081                
30082                
30084                
30085                
30086                
30087                
30088                
30089                
30090                
30091                
30092                
30093                
30094                
30095                
30097                
30098                
30099                
30100                
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30102                
30103                
30104                
30105                
30106                
30107                
30108                
30109                
30110                
30111                
30112                
30113                
30114                
30115                
30116                
30117                
30118                
30119                
30120                
30121                
30122                
30123                
30124                
30125                
30126                
30127                
30128                
30130                
30131                
30132                
30133                
30134                
30135                
30136                
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30145                
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30148                
30149                
30150                
30151                
30152                
30153                
30154                
30155                
30156                
30157                
30158                
30159                
30160                
30162                
30163                
30164                
30165                
30166                
30167                
30168                
30169                
30170                
30171                
30172                
30173                
30174                
30175                
30176                
30177                
30178                
30179                
30180                
30181                
30182                
30183                
30184                
30185                
30187                
30188                
30189                
30190                
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30192                
30193                
30194                
30195                
30196                
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30198                
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30200                
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30202                
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30207                
30208                
30209                
30210                
                 
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 382014-05-16 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 53 to 53
 
091113
091213
Changed:
<
<
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes      
29807                
29808                
29809                
29811                
29812                
29813                
29814                
29815                
29818                
29820                
29821                
29822                
29823                
29824                
29825                
29826                
29827                
29828                
29829                
29832                
29834                
29835                
29837                
29838                
29839                
29840                
29841                
29845                
29846                
29847                
29848                
29849                
29851                
29852                
29853                
29854                
29855                
29859                
29862                
29874                
29875                
29876                
29877                
29878                
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes  
29880 08/19/13   Werner/ Ramona Yes No Yes Yes  
29881 08/19/13   Werner/ Ramona No Yes Yes Yes  
29882 08/19/13   Werner/ Ramona Yes No Yes Yes  
29883     Werner/ Ramona Yes Yes Yes Yes  
29884     Werner/ Ramona Yes Yes Yes Yes  
29885     Werner/ Ramona Yes Yes Yes Yes  
29890                
29891                
29892                
29893                
29894                
29895                
29896                
29897                
29898                
29899                
29901                
29902                
29904     Pierre/ Ramona No No No No  
29905     Pierre/ Ramona No No No No  
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909     Ramona/ Pierre Yes Yes Yes Yes  
29910     Ramona/ Pierre No Yes Yes Yes  
29911                
29912                
29914                
29915                
29916                
29917     Ramona No Yes Yes Yes  
29918                
29919                
29920 08/20/13   Werner          
29921                
29922                
29923                
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925                
29926                
29927                
29928     Ramona No Yes Yes Yes  
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
29930                
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
29932                
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
29934                
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes  
29936                
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes  
29938                
29939                
29940                
29941                
29942                
29943                
29944                
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
29946                
29947                
29948                
29949                
29951                
29952                
29953                
29954                
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
29956                
29957                
29958 08/21/13   Ramona No Yes Yes Yes  
29959                
29960 08/21/13   Ramona No Yes Yes Yes  
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
29966 08/22/13   Ramona No Yes Yes Yes  
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s
29972 08/22/13   Ramona No Yes Yes Yes  
29974                
29975     Ramona No Yes Yes Yes  
29976     Ramona No Yes Yes Yes  
29978                
29980     Ramona No Yes Yes Yes  
29981                
29982                
29983                
29984                
29985                
29986                
29987                
29988                
29989                
29991                
29992                
29993                
29994                
30024                
30025                
30026                
30028                
30029                
30030                
30031                
30032                
30034                
30035                
30036                
30037                
30038                
30039                
30040                
30041                
30042                
30043                
30044                
30045                
30047                
30048                
30049                
30050                
30051                
30052                
30053                
30054                
30055                
30056                
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30160                
30162                
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30168                
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30188                
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30190                
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30192                
30193                
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30195                
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30198                
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30200                
30201                
30202                
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30210                
                 
>
>
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes
29807
29808
29809
29811
29812
29813
29814
29815
29818
29820
29821
29822
29823
29824
29825
29826
29827
29828
29829
29832
29834
29835
29837
29838
29839
29840
29841
29845
29846
29847
29848
29849
29851
29852
29853
29854
29855
29859
29862
29874
29875
29876
29877
29878
29879 08/19/13 Werner/ Ramona Yes Yes Yes Yes
29880 08/19/13 Werner/ Ramona Yes No Yes Yes
29881 08/19/13 Werner/ Ramona No Yes Yes Yes
29882 08/19/13 Werner/ Ramona Yes No Yes Yes
29883 Werner/ Ramona Yes Yes Yes Yes
29884 Werner/ Ramona Yes Yes Yes Yes
29885 Werner/ Ramona Yes Yes Yes Yes
29890
29891
29892
29893
29894
29895
29896
29897
29898
29899
29901
29902
29904 Pierre/ Ramona No No No No
29905 Pierre/ Ramona No No No No
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No Ch0: This channel does not exhibit any charged particle peaks
29909 Ramona/ Pierre Yes Yes Yes Yes
29910 Ramona/ Pierre No Yes Yes Yes
29911
29912
29914
29915
29916
29917 Ramona No Yes Yes Yes
29918
29919
29920 08/20/13 Werner
29921
29922
29923
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925
29926
29927
29928 Ramona No Yes Yes Yes
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
29930
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes
29932
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
29934
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes
29936
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes
29938
29939
29940
29941
29942
29943
29944
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
29946
29947
29948
29949
29951
29952
29953
29954
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
29956
29957
29958 08/21/13 Ramona No Yes Yes Yes
29959
29960 08/21/13 Ramona No Yes Yes Yes
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
29966 08/22/13 Ramona No Yes Yes Yes
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes Ch1: There is only noise after t = .286s
29972 08/22/13 Ramona No Yes Yes Yes
29974
29975 Ramona No Yes Yes Yes
29976// Ramona No Yes Yes Yes
29978
29980 Ramona No Yes Yes Yes
29981
29982
29983
29984
29985
29986
29987
29988
29989
29991
29992
29993
29994
30024 09/04/13

30024_0.5_0.data

30024_0.5_1.data

30024_0.5_2.data

30024_0.5_3.data

 Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
30025 09/04/13

30025_0.5_1.data

30025_0.5_1.data

30025_0.5_2.data

30025_0.5_3.data

Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
30026 09/04/13

30026_0.5_0.data

30026_0.5_1.data

30026_0.5_2.data

30026_0.5_3.data

 Omar Yes Yes Yes Yes All channels had short burts of "overloads" (No registered data). These are very apparent between 200 and 300 ms.
30028 09/04/13

30028_0.5_0.data

30028_0.5_1.data

30028_0.5_2.data

30028_0.5_3.data

 Omar No No No No All channels were either composed of noise or had too much noise for a successful analysis.
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 372014-05-14 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 83 to 83
 
29840                
29841                
29845                
Changed:
<
<
29846     Pierre          
>
>
29846                
 
29847                
29848                
29849                

Revision 362014-05-14 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 83 to 83
 
29840                
29841                
29845                
Changed:
<
<
29846                
>
>
29846     Pierre          
 
29847                
29848                
29849                

Revision 352014-05-14 - jlatorre1513

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 146 to 146
 
29930                
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
29932                
Changed:
<
<
29933                
>
>
29933 08/21/13

29933_0.5_0.data

29933_0.5_1.data

29933_0.5_2.data

29933_0.5_3.data

 Javiera No No No No Every channel was only noise
 
29934                
Changed:
<
<
29935                
>
>
29935 08/21/13

29935_0.5_0.data

29935_0.5_1.data

29935_0.5_2.data

29935_0.5_3.data

 Javiera No Yes Yes Yes  
 
29936                
Changed:
<
<
29937                
>
>
29937 08/21/13

29937_0.5_0.data

29937_0.5_1.data

29937_0.5_2.data

29937_0.5_3.data

 Javiera Yes Yes Yes Yes  
 
29938                
29939                
29940                
Line: 158 to 158
 
29942                
29943                
29944                
Changed:
<
<
29945                
>
>
29945 08/21/13

29945_0.5_0.data

29945_0.5_1.data

29945_0.5_2.data

29945_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: This channel was basically noise but there were 3 peaks that reached past 1 V

Ch1, Ch2, Ch3: useful between t = .1 and t= ,3
 
29946                
29947                
29948                
Line: 167 to 167
 
29952                
29953                
29954                
Changed:
<
<
29955                
>
>
29955 08/21/13

29955_0.5_0.data

29955_0.5_1.data

29955_0.5_2.data

29955_0.5_3.data

 Javiera No Yes Yes Yes Every channel had a very large peak at around t = .382 s. Each of the peaks reached between 2 and 3 volts
 
29956                
29957                
29958 08/21/13   Ramona No Yes Yes Yes  
29959                
29960 08/21/13   Ramona No Yes Yes Yes  
Changed:
<
<
29961                
29962                
29963                
29964                
>
>
29961 08/21/13

29961_0.5_0.data

29961_0.5_1.data

29961_0.5_2.data

29961_0.5_3.data

 Javiera Yes Yes Yes Yes Ch1, Ch2, Ch3: Each channel had a peak at ~ 3 V at t= .356s
29962 08/22/13

29962_0.5_0.data

29962_0.5_1.data

29962_0.5_2.data

29962_0.5_3.data

 Javiera No No No No Every channel was only noise
29963 08/22/13

29963_0.5_0.data

29963_0.5_1.data

29963_0.5_2.data

29963_0.5_3.data

 Javiera No No No No Every channel was only noise
29964 08/22/13

29964_0.5_0.data

29964_0.5_1.data

29964_0.5_2.data

29964_0.5_3.data

 Javiera No Yes Yes Yes

Ch0: Only noise

Ch1, Ch2, Ch3: each one has good data from t = .1s to .3s
 
29966 08/22/13   Ramona No Yes Yes Yes  
Changed:
<
<
29969                
29970                
29971                
>
>
29969 08/22/13

29969_0.5_0.data

29969_0.5_1.data

29969_0.5_2.data

29969_0.5_3.data

 Javiera No No No No

Ch0: Possible overload from t = .282s to t = .288s. Everything else was noise

Ch1: Possible overload from t = .280s to t = .320s. Everything else was noise
29970 08/22/13

29970_0.5_0.data

29970_0.5_1.data

29970_0.5_2.data

29970_0.5_3.data

 Javiera Yes Yes Yes Yes

Ch0: There is some noise from t = .240s to .254s and then again at t = .320s and .330s

Ch1: This channel has a possible overload and useful data from t = .240s to .310s

Ch2, Ch3: both channels had useful data from t = .240s to .320s
29971 08/22/13

29971_0.5_0.data

29971_0.5_1.data

 Javiera No Yes     Ch1: There is only noise after t = .286s
 
29972 08/22/13   Ramona No Yes Yes Yes  
29974                
29975     Ramona No Yes Yes Yes  

Revision 342014-05-13 - Pavila

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 54 to 54
 
091213

Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
Changed:
<
<
29806                
>
>
29806  

29806_0.5_0.data

29806_0.5_1.data

29806_0.5_2.data

29806_0.5_3.data

 Pierre No Yes      
 
29807                
29808                
29809                

Revision 332014-05-10 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 99 to 99
 
29876                
29877                
29878                
Changed:
<
<
29879 08/19/13   Werner Yes Yes Yes Yes  
29880 08/19/13   Werner          
29881 08/19/13   Werner          
29882 08/19/13   Werner          
29883     Werner          
29884     Werner          
29885     Werner          
>
>
29879 08/19/13   Werner/ Ramona Yes Yes Yes Yes  
29880 08/19/13   Werner/ Ramona Yes No Yes Yes  
29881 08/19/13   Werner/ Ramona No Yes Yes Yes  
29882 08/19/13   Werner/ Ramona Yes No Yes Yes  
29883     Werner/ Ramona Yes Yes Yes Yes  
29884     Werner/ Ramona Yes Yes Yes Yes  
29885     Werner/ Ramona Yes Yes Yes Yes  
 
29890                
29891                
29892                
Line: 118 to 118
 
29899                
29901                
29902                
Changed:
<
<
29904     Pierre          
29905     Pierre          
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar Yes Yes    

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre No Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre and Ramona No       Ch0: This channel does not exhibit any charged particle peaks
29909     Pierre          
29910     Pierre          
>
>
29904     Pierre/ Ramona No No No No  
29905     Pierre/ Ramona No No No No  
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar/ Ramona Yes Yes Yes Yes

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre/ Ramona Yes Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909     Ramona/ Pierre Yes Yes Yes Yes  
29910     Ramona/ Pierre No Yes Yes Yes  
 
29911                
29912                
29914                
29915                
29916                
Changed:
<
<
29917     Ramona          
>
>
29917     Ramona No Yes Yes Yes  
 
29918                
29919                
29920 08/20/13   Werner          
29921                
29922                
29923                
Changed:
<
<
29924 08/20/13 29924_0.5_0.data Omar and Ramona No       Ch0: This channel is very noisy. Very few peaks have noisless bases.
>
>
29924 08/20/13 29924_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is very noisy. Very few peaks have noisless bases.
 
29925                
29926                
29927                
Changed:
<
<
29928     Ramona          
29929 08/20/13 29929_0.5_0.data Omar and Ramona No       Ch0: This channel is almost all noise.
>
>
29928     Ramona No Yes Yes Yes  
29929 08/20/13 29929_0.5_0.data Ramona/ Omar No Yes Yes Yes Ch0: This channel is almost all noise.
 
29930                
29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
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29958 08/21/13   Ramona No Yes Yes Yes  
 
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29960 08/21/13   Ramona          
>
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29960 08/21/13   Ramona No Yes Yes Yes  
 
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29966 08/22/13   Ramona          
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29966 08/22/13   Ramona No Yes Yes Yes  
 
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29972 08/22/13   Ramona No Yes Yes Yes  
 
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29975     Ramona No Yes Yes Yes  
29976     Ramona No Yes Yes Yes  
 
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29980     Ramona No Yes Yes Yes  
 
29981                
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Revision 322014-04-23 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 12 to 12
 
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3
Changed:
<
<
  • Note that for the shot_list_old.data, the RP values indicate the distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are the input values to the RP control box during data collection
>
>
  • Note that for the shot_list.data on nyoko2, the setpoint values are the input values to the RP control box during data collection
 Figure Set 1: Detector Positions

Figure Set 2: Channel Particle Trajectories

Revision 312014-04-08 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 104 to 104
 
29880 08/19/13   Werner          
29881 08/19/13   Werner          
29882 08/19/13   Werner          
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29883     Werner          
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29904     Pierre          
29905     Pierre          
 
29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar Yes Yes    

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre No Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
Changed:
<
<
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909                
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>
>
29908 08/20/13 29908_0.5_0.data Pierre and Ramona No       Ch0: This channel does not exhibit any charged particle peaks
29909     Pierre          
29910     Pierre          
 
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29917     Ramona          
 
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29920 08/20/13   Werner          
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Changed:
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29924 08/20/13 29924_0.5_0.data Omar No       Ch0: This channel is very noisy. Very few peaks have noisless bases.
>
>
29924 08/20/13 29924_0.5_0.data Omar and Ramona No       Ch0: This channel is very noisy. Very few peaks have noisless bases.
 
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29929 08/20/13 29929_0.5_0.data Omar No       Ch0: This channel is almost all noise.
>
>
29928     Ramona          
29929 08/20/13 29929_0.5_0.data Omar and Ramona No       Ch0: This channel is almost all noise.
 
29930                
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29931 08/20/13

29931_0.5_0.data

29931_0.5_1.data

29931_0.5_2.data

29931_0.5_3.data

 Ramona No Yes Yes Yes  
 
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Revision 302014-04-02 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 26 to 26
 
Data Log
Changed:
<
<

Scenario Shots

>
>		Scenario Shots
 
Scenario: Reference Shots

     
Beam Blip/ NBI Slowing Down 29958 29960 29966 29972 - -
Quiescent MHD 29904 29905 29906 29908 29909 29910
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091113
091213
Changed:
<
<
Shot Date Shot # Filename "ctrl_fm_" + /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
20/08/13 29924 29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
08/19/13 29879     Werner Yes       Sawteeth

08/19/13 29879     Werner   Yes     Sawteeth  
08/19/13 29879     Werner     Yes   Sawteeth  
08/19/13 29879     Werner       Yes Sawteeth  
08/20/13 29906 29906_0.5_1.data /DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
>
>
Shot # Shot Date Filename "ctrl_fm_" + Investigator Ch0 Ch1 Ch2 Ch3 Notes
29806                
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29879 08/19/13   Werner Yes Yes Yes Yes  
29880 08/19/13   Werner          
29881 08/19/13   Werner          
29882 08/19/13   Werner          
29883                
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29906 08/20/13 29906_0.5_0.data

29906_0.5_1.data

 Omar Yes Yes    

Ch0: There was only noise after 0.3 seconds.

Ch1: This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
29907 08/20/13 29907_0.5_0.data Pierre No Yes Yes Yes Ch3: Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
29908 08/20/13 29908_0.5_0.data Pierre No       Ch0: This channel does not exhibit any charged particle peaks
29909                
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29920 08/20/13   Werner          
29921                
29922                
29923                
29924 08/20/13 29924_0.5_0.data Omar No       Ch0: This channel is very noisy. Very few peaks have noisless bases.
29925                
29926                
29927                
29928                
29929 08/20/13 29929_0.5_0.data Omar No       Ch0: This channel is almost all noise.
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29958 08/21/13   Ramona          
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29966 08/22/13   Ramona          
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29972 08/22/13   Ramona          
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META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 292014-03-29 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 12 to 12
 
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3
Changed:
<
<
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
>
>
  • Note that for the shot_list_old.data, the RP values indicate the distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are the input values to the RP control box during data collection
 Figure Set 1: Detector Positions

Figure Set 2: Channel Particle Trajectories

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    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Changed:
<
<

Figure Set 1: Detector Positions

Figure Set 2: Channel Particle Trajectories

Figure Set 3: PD Offsets from RP

>
>		Figure Set 1: Detector Positions
 
Changed:
<
<
Figure Set 4: Detector Angular Orientations

Data Log

>
>		 Figure Set 2: Channel Particle Trajectories

Figure Set 3: PD Offsets from RP

Figure Set 4: Detector Angular Orientations

Data Log

 

Scenario Shots

Scenario: Reference Shots

     
Beam Blip/ NBI Slowing Down 29958 29960 29966 29972 - -

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 17 to 17
 
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection

Figure Set 1: Detector Positions

Deleted:
<
<		 A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3. The entrance of the collimators leading to each detector is visible in the image.

detector_orientation_imagelabled2.png

B. An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.

Origin3_scaledlabeled2.png

 

Figure Set 2: Channel Particle Trajectories

Deleted:
<
<		 Graphical orbit particle trajectory output from FEPP's modified Orbit Code:

A. (Left) Plasma/ tokamak poloidal cross section particle trajectories, the black arrows represent particle trajectories ending at the detectors (Right) Plasma/ tokamak toroidal cross section particle trajectories, the black arrows represent particle trajectories ending at the detectors

Ramona_image1_scaledlabeled.png

B. (Left) Magnification of the plasma/ tokamak poloidal cross section particle trajectories, view C for details inside black box (Right) Magnification of the plasma/ tokamak toroidal cross section particle trajectories, view C for details inside black box

Ramona_image2_croppedlabeled.png

C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section

Ramona_image3_scaledlabeled2.png

 

Figure Set 3: PD Offsets from RP

Changed:
<
<		A. (TOP) The PD probe head's porthole of the tokamak, as well as the central axis of the reciprocating probe arm, lies along the R-axis. The base of the RP has its center or origin as indicated. All PD Channel collimator entrance offsets are measured from this origin. (BOTTOM) The base of the RP lies along the R-axis.

Origin1_scaledlabeled2.png

Origin2labeled.png

B. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The horizontal displacements along the R-axis between the entrance of each Channel's collimator to the base of the RP (as defined in Figure Set 3.A.).

Radial_offset2_scaledlabeled_2.png

Radial_offset1labeled2.png

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 R: 149.78mm
1 1 R: 120.97mm
2 2 R: 128.65mm
3 3 R: 140.69mm

C. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The vertical displacements along the Z-axis between the entrance of each Channel's collimator to the R-axis.

Radial_offset2_scaledlabeled_2.png

Vertical_offset1labeled2.PNG

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 Z: 25.8mm
1 1 Z: 30.64mm
2 2 Z: 39.06mm
3 3 Z: 14.32mm

D. (TOP) Looking at the toroidal cross section of the tokamak, on top of the PD head yields the following Y-axis and R-axis, with the Z-axis coming out of the page. (BOTTOM) The horizontal displacements along the Y-axis between the entrance of each Channel's collimator to the R-axis.

Horizontal_offset4_scaledlabeled_2.png

Horizontal_offset1labeled2.png

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 Y: 27.49mm
1 1 Y: 31.11mm
2 2 Y: 14.62mm
3 3 Y: 41.59mm

Figure Set 4: Detector Angular Orientations

This figure repesents the detector angular orientations (phi, theta), in which the coordinate system is displaced and parallel to the MAST tokamak coordinate system. The MAST tokamak's coordinate system has the origin of its coordinate system placed in the center of the tokamak (which lies along the negative x-axis).

detector_geometry1.png

>
>
Figure Set 4: Detector Angular Orientations
 

Data Log

Scenario Shots

Scenario: Reference Shots

     

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 16 to 16
 
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Changed:
<
<

Figure Set 1: Detector Positions

>
>

Figure Set 1: Detector Positions

  A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3. The entrance of the collimators leading to each detector is visible in the image.
Line: 26 to 26
  Origin3_scaledlabeled2.png
Changed:
<
<

Figure Set 2: Channel Particle Trajectories

>
>

Figure Set 2: Channel Particle Trajectories

  Graphical orbit particle trajectory output from FEPP's modified Orbit Code:
Line: 41 to 41
 C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section

Ramona_image3_scaledlabeled2.png

Changed:
<
<

Figure Set 3: PD Offsets from RP

>
>

Figure Set 3: PD Offsets from RP

  A. (TOP) The PD probe head's porthole of the tokamak, as well as the central axis of the reciprocating probe arm, lies along the R-axis. The base of the RP has its center or origin as indicated. All PD Channel collimator entrance offsets are measured from this origin. (BOTTOM) The base of the RP lies along the R-axis.
Line: 81 to 81
 
1 1 Y: 31.11mm
2 2 Y: 14.62mm
3 3 Y: 41.59mm
Changed:
<
<

Figure Set 4: Detector Angular Orientations

>
>

Figure Set 4: Detector Angular Orientations

  This figure repesents the detector angular orientations (phi, theta), in which the coordinate system is displaced and parallel to the MAST tokamak coordinate system. The MAST tokamak's coordinate system has the origin of its coordinate system placed in the center of the tokamak (which lies along the negative x-axis).

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 99 to 99
 
Scenario: Non-Resonant Perturbations Shots

       
Sawteeth 29879 29880 29881 29882 29883 29884 29885

Shot Log

Changed:
<
<
Shot Date
081513


>
>
Shot Date
080513
081613
081913
082013
082113
082213
082313
090413
090513
090613
090913
091013
091113
091213
 
Shot Date Shot # Filename "ctrl_fm_" + /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks

Revision 242014-02-26 - aangu003

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 16 to 16
 
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Deleted:
<
<
 

Figure Set 1: Detector Positions

A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3. The entrance of the collimators leading to each detector is visible in the image.

Line: 100 to 99
 
Scenario: Non-Resonant Perturbations Shots

       
Sawteeth 29879 29880 29881 29882 29883 29884 29885

Shot Log

Added:
>
>
Shot Date
081513


 
Shot Date Shot # Filename "ctrl_fm_" + /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)

Revision 232014-02-26 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 102 to 102
 

Shot Log

Shot Date Shot # Filename "ctrl_fm_" + /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
Changed:
<
<
20/08/13 29907 29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot is not quiescent (See Mirnov and Fission Chamber Data) *: CH 3 is a nice signal but is unable to generate rates
>
>
20/08/13 29907 29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot first thought to be quiescent but is not (See Mirnov and Fission Chamber Data)
 
20/08/13 29924 29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.

Revision 222014-02-19 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
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Back to MAST Diagnostic

Line: 16 to 16
 
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Added:
>
>
 

Figure Set 1: Detector Positions

A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3. The entrance of the collimators leading to each detector is visible in the image.

Revision 212014-02-12 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<

Data Channel #

Detector Positions

Angular Orientation

Trajectory Color

Detector Collimator Entrance Offset from RP

  
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm  
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm  
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm  
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm  
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3  
>
>

Data Channel #

Detector Positions

Angular Orientation

Trajectory Color

Detector Collimator Entrance Offset from RP
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3
 
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
Line: 54 to 54
 Radial_offset2_scaledlabeled_2.png

Radial_offset1labeled2.png

Added:
>
>

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 R: 149.78mm
1 1 R: 120.97mm
2 2 R: 128.65mm
3 3 R: 140.69mm
  C. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The vertical displacements along the Z-axis between the entrance of each Channel's collimator to the R-axis.

Radial_offset2_scaledlabeled_2.png

Vertical_offset1labeled2.PNG

Added:
>
>

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 Z: 25.8mm
1 1 Z: 30.64mm
2 2 Z: 39.06mm
3 3 Z: 14.32mm
  D. (TOP) Looking at the toroidal cross section of the tokamak, on top of the PD head yields the following Y-axis and R-axis, with the Z-axis coming out of the page. (BOTTOM) The horizontal displacements along the Y-axis between the entrance of each Channel's collimator to the R-axis.

Horizontal_offset4_scaledlabeled_2.png

Horizontal_offset1labeled2.png

Added:
>
>

Data Channel #

Detector Positions

Detector Collimator Entrance Offset from RP
0 4 Y: 27.49mm
1 1 Y: 31.11mm
2 2 Y: 14.62mm
3 3 Y: 41.59mm
 

Figure Set 4: Detector Angular Orientations

This figure repesents the detector angular orientations (phi, theta), in which the coordinate system is displaced and parallel to the MAST tokamak coordinate system. The MAST tokamak's coordinate system has the origin of its coordinate system placed in the center of the tokamak (which lies along the negative x-axis).

detector_geometry1.png

Data Log

Changed:
<
<
Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot is not quiescent (See Mirnov and Fission Chamber Data) *: CH 3 is a nice signal but is unable to generate rates
20/08/13 29924 ctrl_fm_29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 ctrl_fim_29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
>
>

Scenario Shots

Scenario: Reference Shots

     
Beam Blip/ NBI Slowing Down 29958 29960 29966 29972 - -
Quiescent MHD 29904 29905 29906 29908 29909 29910

Scenario: Resonant Perturbations Shots

     
Low Amplitude MHD 29917 29924 29928 29929 29931
Large Amplitude Fishbones 29975 29976 29980 - -

Scenario: Non-Resonant Perturbations Shots

       
Sawteeth 29879 29880 29881 29882 29883 29884 29885

Shot Log

Shot Date Shot # Filename "ctrl_fm_" + /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot is not quiescent (See Mirnov and Fission Chamber Data) *: CH 3 is a nice signal but is unable to generate rates
20/08/13 29924 29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
 
08/19/13 29879     Werner Yes       Sawteeth

08/19/13 29879     Werner   Yes     Sawteeth  
08/19/13 29879     Werner     Yes   Sawteeth  
08/19/13 29879     Werner       Yes Sawteeth  
Changed:
<
<
08/20/13 29906 ctrl_fm_29906_0.5_1.data /DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
>
>
08/20/13 29906 29906_0.5_1.data /DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
 
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
Line: 126 to 152
 
                     
                     
                     
Deleted:
<
<
                     
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 202014-02-12 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 75 to 75
 
Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
Changed:
<
<
20/08/13 29907 ctrl_fm_29907_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
>
>
20/08/13 29907 ctrl_fm_29907_0.5_0.data /DataLog/QuiescentShots Pierre No Yes Yes Yes* Quiescent Plasma Shot is not quiescent (See Mirnov and Fission Chamber Data) *: CH 3 is a nice signal but is unable to generate rates
 
20/08/13 29924 ctrl_fm_29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 ctrl_fim_29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.

Revision 192014-02-11 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 10 to 10
 
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm  
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm  
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm  
Changed:
<
<
Figure Set 1 Figure Set 1 Figure Set __ Figure Set 2 Figure Set 3  
>
>
Figure Set 1 Figure Set 1 Figure Set 4 Figure Set 2 Figure Set 3  
 
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
Line: 18 to 18
 
    • the input value to the RP control box during data collection

Figure Set 1: Detector Positions

Changed:
<
<		A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3.
>
>		A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3. The entrance of the collimators leading to each detector is visible in the image.
  detector_orientation_imagelabled2.png
Line: 49 to 49
  Origin2labeled.png
Changed:
<
<		B. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The horizontal displacements along the R-axis between the entrance of each Channel's collimator to the base of the RP (as defined in Figure 3.A.).
>
>		B. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The horizontal displacements along the R-axis between the entrance of each Channel's collimator to the base of the RP (as defined in Figure Set 3.A.).
  Radial_offset2_scaledlabeled_2.png
Line: 66 to 66
 Horizontal_offset4_scaledlabeled_2.png

Horizontal_offset1labeled2.png

Added:
>
>

Figure Set 4: Detector Angular Orientations

This figure repesents the detector angular orientations (phi, theta), in which the coordinate system is displaced and parallel to the MAST tokamak coordinate system. The MAST tokamak's coordinate system has the origin of its coordinate system placed in the center of the tokamak (which lies along the negative x-axis).

detector_geometry1.png

 

Data Log

Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Line: 149 to 154
 
META FILEATTACHMENT attachment="Vertical_offset1labeled2.PNG" attr="h" comment="" date="1392144032" name="Vertical_offset1labeled2.PNG" path="Vertical_offset1labeled2.PNG" size="92819" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Horizontal_offset4_scaledlabeled_2.png" attr="h" comment="" date="1392144894" name="Horizontal_offset4_scaledlabeled_2.png" path="Horizontal_offset4_scaledlabeled_2.png" size="150557" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset2_scaledlabeled_2.png" attr="h" comment="" date="1392144893" name="Radial_offset2_scaledlabeled_2.png" path="Radial_offset2_scaledlabeled_2.png" size="155181" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="detector_geometry.pdf" attr="h" comment="" date="1392153770" name="detector_geometry.pdf" path="detector_geometry.pdf" size="52093" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_geometry1.png" attr="h" comment="" date="1392153916" name="detector_geometry1.png" path="detector_geometry1.png" size="73423" user="lc_2eramona" version="1"

Revision 182014-02-11 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<

Data

Channel #

Detector Positions

(Figure Set 1)

Angular Orientation

(Figure Set _)

Trajectory Color

(Figure Set 2)

Detector Collimator Entrance Offset from RP

Figure Set 3
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
>
>

Data Channel #

Detector Positions

Angular Orientation

Trajectory Color

Detector Collimator Entrance Offset from RP

  
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm  
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm  
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm  
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm  
Figure Set 1 Figure Set 1 Figure Set __ Figure Set 2 Figure Set 3  
 
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
Line: 19 to 20
  A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3.
Changed:
<
<		detector_orientation_image.jpg
>
>		detector_orientation_imagelabled2.png
 
Changed:
<
<		B. An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.
>
>		B. An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.
 
Changed:
<
<		Origin3_scaledlabeled.png
>
>		Origin3_scaledlabeled2.png
 

Figure Set 2: Channel Particle Trajectories

Line: 39 to 40
  C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section
Changed:
<
<		Ramona_image3_scaledlabeled.png
>
>		Ramona_image3_scaledlabeled2.png
 

Figure Set 3: PD Offsets from RP

A. (TOP) The PD probe head's porthole of the tokamak, as well as the central axis of the reciprocating probe arm, lies along the R-axis. The base of the RP has its center or origin as indicated. All PD Channel collimator entrance offsets are measured from this origin. (BOTTOM) The base of the RP lies along the R-axis.

Changed:
<
<		Origin1_scaledlabeled.png
>
>		Origin1_scaledlabeled2.png
 
Changed:
<
<		Origin2_labeled.png
>
>		Origin2labeled.png
  B. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The horizontal displacements along the R-axis between the entrance of each Channel's collimator to the base of the RP (as defined in Figure 3.A.).
Changed:
<
<		Radial_offset2_scaledlabeled.png
>
>		Radial_offset2_scaledlabeled_2.png
 
Changed:
<
<		Radial_offset1labeled.png
>
>		Radial_offset1labeled2.png
  C. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The vertical displacements along the Z-axis between the entrance of each Channel's collimator to the R-axis.
Changed:
<
<		Radial_offset2_scaledlabeled.png
>
>		Radial_offset2_scaledlabeled_2.png
 
Changed:
<
<		Vertical_offset1labeled.png
>
>		Vertical_offset1labeled2.PNG
  D. (TOP) Looking at the toroidal cross section of the tokamak, on top of the PD head yields the following Y-axis and R-axis, with the Z-axis coming out of the page. (BOTTOM) The horizontal displacements along the Y-axis between the entrance of each Channel's collimator to the R-axis.
Changed:
<
<		Horizontal_offset4_scaledlabeled.png
>
>		Horizontal_offset4_scaledlabeled_2.png
 
Changed:
<
<		Horizontal_offset1labeled.png
>
>		Horizontal_offset1labeled2.png
 

Data Log

Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Line: 138 to 139
 
META FILEATTACHMENT attachment="Radial_offset1labeled.png" attr="h" comment="" date="1392102526" name="Radial_offset1labeled.png" path="Radial_offset1labeled.png" size="91191" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset2_scaledlabeled.png" attr="h" comment="" date="1392102526" name="Radial_offset2_scaledlabeled.png" path="Radial_offset2_scaledlabeled.png" size="152506" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Vertical_offset1labeled.png" attr="h" comment="" date="1392102525" name="Vertical_offset1labeled.png" path="Vertical_offset1labeled.png" size="128775" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="detector_orientation_imagelabled2.png" attr="h" comment="" date="1392144042" name="detector_orientation_imagelabled2.png" path="detector_orientation_imagelabled2.png" size="379373" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Horizontal_offset1labeled2.png" attr="h" comment="" date="1392144040" name="Horizontal_offset1labeled2.png" path="Horizontal_offset1labeled2.png" size="93686" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin1_scaledlabeled2.png" attr="h" comment="" date="1392144039" name="Origin1_scaledlabeled2.png" path="Origin1_scaledlabeled2.png" size="262932" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin2labeled.png" attr="h" comment="" date="1392144038" name="Origin2labeled.png" path="Origin2labeled.png" size="165645" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin3_scaledlabeled2.png" attr="h" comment="" date="1392144038" name="Origin3_scaledlabeled2.png" path="Origin3_scaledlabeled2.png" size="418801" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset1labeled2.png" attr="h" comment="" date="1392144035" name="Radial_offset1labeled2.png" path="Radial_offset1labeled2.png" size="91813" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image3_scaledlabeled2.png" attr="h" comment="" date="1392144034" name="Ramona_image3_scaledlabeled2.png" path="Ramona_image3_scaledlabeled2.png" size="306211" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Vertical_offset1labeled2.PNG" attr="h" comment="" date="1392144032" name="Vertical_offset1labeled2.PNG" path="Vertical_offset1labeled2.PNG" size="92819" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Horizontal_offset4_scaledlabeled_2.png" attr="h" comment="" date="1392144894" name="Horizontal_offset4_scaledlabeled_2.png" path="Horizontal_offset4_scaledlabeled_2.png" size="150557" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset2_scaledlabeled_2.png" attr="h" comment="" date="1392144893" name="Radial_offset2_scaledlabeled_2.png" path="Radial_offset2_scaledlabeled_2.png" size="155181" user="lc_2eramona" version="1"

Revision 172014-02-11 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<
Channel # Detector Position Angular Orientation Trajectory Color Detector Collimator Entrance Offset from RP
0 4 (Figure 1) Phi -45deg, Theta 40deg Yellow (Figure 2) R: 149.78mm, Z: 25.8mm, Y: 27.49mm (Figure 3)
1 1 (Figure 1) Phi -30deg, Theta 40deg Red (Figure 2) R: 120.97mm, Z: 30.64mm, Y: 31.11mm (Figure 3)
2 2 (Figure 1) Phi -35deg, Theta 40deg Green (Figure 2) R: 128.65mm, Z: 39.06mm, Y: 14.62mm (Figure 3)
3 3 (Figure 1) Phi -40deg, Theta 40deg Blue (Figure 2) R: 140.69mm, Z: 14.32mm, Y: 41.59mm (Figure 3)
>
>

Data

Channel #

Detector Positions

(Figure Set 1)

Angular Orientation

(Figure Set _)

Trajectory Color

(Figure Set 2)

Detector Collimator Entrance Offset from RP

Figure Set 3
0 4 Phi -45deg, Theta 40deg Yellow R: 149.78mm, Z: 25.8mm, Y: 27.49mm
1 1 Phi -30deg, Theta 40deg Red R: 120.97mm, Z: 30.64mm, Y: 31.11mm
2 2 Phi -35deg, Theta 40deg Green R: 128.65mm, Z: 39.06mm, Y: 14.62mm
3 3 Phi -40deg, Theta 40deg Blue R: 140.69mm, Z: 14.32mm, Y: 41.59mm
 
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Changed:
<
<

Figure 1: Detector Positions

>
>

Figure Set 1: Detector Positions

  A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3.

detector_orientation_image.jpg

Changed:
<
<		B. (TOP) An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale. (BOTTOM) An image of the probe head with the outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.
>
>		B. An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.
  Origin3_scaledlabeled.png
Changed:
<
<		Origin4_scaledlabeled.png

Figure 2: Channel Particle Trajectories

>
>

Figure Set 2: Channel Particle Trajectories

  Graphical orbit particle trajectory output from FEPP's modified Orbit Code:
Line: 41 to 40
 C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section

Ramona_image3_scaledlabeled.png

Changed:
<
<

Figure 3: PD Offsets from RP Connection

>
>

Figure Set 3: PD Offsets from RP

  A. (TOP) The PD probe head's porthole of the tokamak, as well as the central axis of the reciprocating probe arm, lies along the R-axis. The base of the RP has its center or origin as indicated. All PD Channel collimator entrance offsets are measured from this origin. (BOTTOM) The base of the RP lies along the R-axis.

Revision 162014-02-11 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 15 to 15
 
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
Changed:
<
<

Figure 1

>
>

Figure 1: Detector Positions

 
Changed:
<
<		Please note that the original image is courtesy of the CCFE Drawing Office
>
>		A. Note that the original image is courtesy of the CCFE Drawing Office. Channel 0 contains Detector 4, Channel 1 contains Detector 1, Channel 2 contains Detector 2, and Channel 3 contains Detector 3.
  detector_orientation_image.jpg
Changed:
<
<

Figure 2

>
>		 B. (TOP) An image of the probe head with a transparent outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale. (BOTTOM) An image of the probe head with the outer Boron Nitride (BN) shield. Note that the reciprocating probe arm's inner tube length is not drawn to scale.

Origin3_scaledlabeled.png

Origin4_scaledlabeled.png

Figure 2: Channel Particle Trajectories

  Graphical orbit particle trajectory output from FEPP's modified Orbit Code:
Line: 35 to 41
 C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section

Ramona_image3_scaledlabeled.png

Changed:
<
<

Figure 3

>
>

Figure 3: PD Offsets from RP Connection

A. (TOP) The PD probe head's porthole of the tokamak, as well as the central axis of the reciprocating probe arm, lies along the R-axis. The base of the RP has its center or origin as indicated. All PD Channel collimator entrance offsets are measured from this origin. (BOTTOM) The base of the RP lies along the R-axis.

Origin1_scaledlabeled.png

Origin2_labeled.png

B. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The horizontal displacements along the R-axis between the entrance of each Channel's collimator to the base of the RP (as defined in Figure 3.A.).

Radial_offset2_scaledlabeled.png

Radial_offset1labeled.png

C. (TOP) Looking at the poloidal cross section of the tokamak, of the PD head yields the following Z-axis and R-axis, with the Y-axis going into the page. (BOTTOM) The vertical displacements along the Z-axis between the entrance of each Channel's collimator to the R-axis.

Radial_offset2_scaledlabeled.png

Vertical_offset1labeled.png

D. (TOP) Looking at the toroidal cross section of the tokamak, on top of the PD head yields the following Y-axis and R-axis, with the Z-axis coming out of the page. (BOTTOM) The horizontal displacements along the Y-axis between the entrance of each Channel's collimator to the R-axis.

Horizontal_offset4_scaledlabeled.png

 
Changed:
<
<		Image of detector offsets from RP
>
>		Horizontal_offset1labeled.png
 

Data Log

Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Line: 102 to 130
 
META FILEATTACHMENT attachment="Ramona_image1_scaled.png" attr="h" comment="" date="1391844039" name="Ramona_image1_scaled.png" path="Ramona_image1_scaled.png" size="204831" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image2_croppedlabeled.png" attr="h" comment="" date="1391845086" name="Ramona_image2_croppedlabeled.png" path="Ramona_image2_croppedlabeled.png" size="184363" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image1_scaledlabeled.png" attr="h" comment="" date="1391845085" name="Ramona_image1_scaledlabeled.png" path="Ramona_image1_scaledlabeled.png" size="248670" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="Horizontal_offset1labeled.png" attr="h" comment="" date="1392102534" name="Horizontal_offset1labeled.png" path="Horizontal_offset1labeled.png" size="93808" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Horizontal_offset4_scaledlabeled.png" attr="h" comment="" date="1392102534" name="Horizontal_offset4_scaledlabeled.png" path="Horizontal_offset4_scaledlabeled.png" size="146666" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin1_scaledlabeled.png" attr="h" comment="" date="1392102533" name="Origin1_scaledlabeled.png" path="Origin1_scaledlabeled.png" size="260634" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin2_labeled.png" attr="h" comment="" date="1392102531" name="Origin2_labeled.png" path="Origin2_labeled.png" size="163408" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin3_scaledlabeled.png" attr="h" comment="" date="1392102531" name="Origin3_scaledlabeled.png" path="Origin3_scaledlabeled.png" size="411615" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Origin4_scaledlabeled.png" attr="h" comment="" date="1392102528" name="Origin4_scaledlabeled.png" path="Origin4_scaledlabeled.png" size="351138" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset1labeled.png" attr="h" comment="" date="1392102526" name="Radial_offset1labeled.png" path="Radial_offset1labeled.png" size="91191" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Radial_offset2_scaledlabeled.png" attr="h" comment="" date="1392102526" name="Radial_offset2_scaledlabeled.png" path="Radial_offset2_scaledlabeled.png" size="152506" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Vertical_offset1labeled.png" attr="h" comment="" date="1392102525" name="Vertical_offset1labeled.png" path="Vertical_offset1labeled.png" size="128775" user="lc_2eramona" version="1"

Revision 152014-02-11 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 95 to 95
 
                     
                     
Deleted:
<
<
  • Ramona_image2_croppedlabeled.png:

  • Ramona_image1_scaledlabeled.png:
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image2_cropped.png" attr="h" comment="" date="1391843609" name="Ramona_image2_cropped.png" path="Ramona_image2_cropped.png" size="159261" user="lc_2eramona" version="1"

Revision 142014-02-08 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<
Channel # Detector Position Angular Orientation Trajectory Color Detector X (R) Offset from RP Detector Z Offset from RP Detector Y Offset from RP
0 4 (Figure 1) Phi -45deg, Theta 40deg Yellow (Figure 2) cm cm cm
1 1 (Figure 1) Phi -30deg, Theta 40deg Red (Figure 2) cm cm cm
2 2 (Figure 1) Phi -35deg, Theta 40deg Green (Figure 2) cm cm cm
3 3 (Figure 1) Phi -40deg, Theta 40deg Blue (Figure 2) cm cm cm
>
>
Channel # Detector Position Angular Orientation Trajectory Color Detector Collimator Entrance Offset from RP
0 4 (Figure 1) Phi -45deg, Theta 40deg Yellow (Figure 2) R: 149.78mm, Z: 25.8mm, Y: 27.49mm (Figure 3)
1 1 (Figure 1) Phi -30deg, Theta 40deg Red (Figure 2) R: 120.97mm, Z: 30.64mm, Y: 31.11mm (Figure 3)
2 2 (Figure 1) Phi -35deg, Theta 40deg Green (Figure 2) R: 128.65mm, Z: 39.06mm, Y: 14.62mm (Figure 3)
3 3 (Figure 1) Phi -40deg, Theta 40deg Blue (Figure 2) R: 140.69mm, Z: 14.32mm, Y: 41.59mm (Figure 3)
 
  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
Line: 22 to 22
 detector_orientation_image.jpg

Figure 2

Changed:
<
<		Graphical orbit particle trajectory output from FEPP's modified Orbit Code
>
>		Graphical orbit particle trajectory output from FEPP's modified Orbit Code:
 
Added:
>
>		A. (Left) Plasma/ tokamak poloidal cross section particle trajectories, the black arrows represent particle trajectories ending at the detectors (Right) Plasma/ tokamak toroidal cross section particle trajectories, the black arrows represent particle trajectories ending at the detectors

Ramona_image1_scaledlabeled.png

B. (Left) Magnification of the plasma/ tokamak poloidal cross section particle trajectories, view C for details inside black box (Right) Magnification of the plasma/ tokamak toroidal cross section particle trajectories, view C for details inside black box

Ramona_image2_croppedlabeled.png

C. (Left) Magnification of central particle trajectories ending at detectors, poloidal cross section (Right) Magnification of central particle trajectories ending at detectors, toroidal cross section

Ramona_image3_scaledlabeled.png

Figure 3

Image of detector offsets from RP

 

Data Log

Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Line: 81 to 95
 
                     
                     
Added:
>
>
  • Ramona_image2_croppedlabeled.png:

  • Ramona_image1_scaledlabeled.png:
 
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="Ramona_image2_cropped.png" attr="h" comment="" date="1391843609" name="Ramona_image2_cropped.png" path="Ramona_image2_cropped.png" size="159261" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image3_scaledlabeled.png" attr="h" comment="" date="1391843753" name="Ramona_image3_scaledlabeled.png" path="Ramona_image3_scaledlabeled.png" size="225330" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image1_scaled.png" attr="h" comment="" date="1391844039" name="Ramona_image1_scaled.png" path="Ramona_image1_scaled.png" size="204831" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image2_croppedlabeled.png" attr="h" comment="" date="1391845086" name="Ramona_image2_croppedlabeled.png" path="Ramona_image2_croppedlabeled.png" size="184363" user="lc_2eramona" version="1"
META FILEATTACHMENT attachment="Ramona_image1_scaledlabeled.png" attr="h" comment="" date="1391845085" name="Ramona_image1_scaledlabeled.png" path="Ramona_image1_scaledlabeled.png" size="248670" user="lc_2eramona" version="1"

Revision 132014-02-07 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<
Channel # Detector Position in Housing Angular Orientation Orbit Trajectory Color Detector X (R) Offset from RP Detector Z Offset from RP Detector Y Offset from RP
0 4 (labeled in Figure 1) Phi -45deg, Theta 40deg Yellow (see Figure 2) cm cm cm
1 1 (labeled in Figure 1) Phi -30deg, Theta 40deg Red (see Figure 2) cm cm cm
2 2 (labeled in Figure 1) Phi -35deg, Theta 40deg Green (see Figure 2) cm cm cm
3 3 (labeled in Figure 1) Phi -40deg, Theta 40deg Blue (see Figure 2) cm cm cm
>
>
Channel # Detector Position Angular Orientation Trajectory Color Detector X (R) Offset from RP Detector Z Offset from RP Detector Y Offset from RP
0 4 (Figure 1) Phi -45deg, Theta 40deg Yellow (Figure 2) cm cm cm
1 1 (Figure 1) Phi -30deg, Theta 40deg Red (Figure 2) cm cm cm
2 2 (Figure 1) Phi -35deg, Theta 40deg Green (Figure 2) cm cm cm
3 3 (Figure 1) Phi -40deg, Theta 40deg Blue (Figure 2) cm cm cm

  • Note that for the shot_list_old.data, the RP values indicate:
    • distance from the center of the tokamak to the entrance of the collimator for Channel 0 (or to the entrance of the collimator for Detector 4)
  • Note that for the shot_list_new.data, the setpoint values are:
    • the input value to the RP control box during data collection
 

Figure 1

Please note that the original image is courtesy of the CCFE Drawing Office

Line: 17 to 22
 detector_orientation_image.jpg

Figure 2

Changed:
<
<		Graphical particle trajectory output from FEPP's modified Orbit Code
>
>		Graphical orbit particle trajectory output from FEPP's modified Orbit Code
 

Data Log

Changed:
<
<
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
>
>
Shot Date Shot # Filename /data/plasma.1/Digitizer/Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29906 ctrl_fim_29906_0.5_0.data /DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
 
08/19/13 29879     Werner Yes       Sawteeth

08/19/13 29879     Werner   Yes     Sawteeth  
08/19/13 29879     Werner     Yes   Sawteeth  
08/19/13 29879     Werner       Yes Sawteeth  
Changed:
<
<
08/20/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
>
>
08/20/13 29906 ctrl_fm_29906_0.5_1.data /DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
 
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  

Revision 122014-02-05 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Line: 6 to 6
 

Detector Orientations

Channel # Detector Position in Housing Angular Orientation Orbit Trajectory Color Detector X (R) Offset from RP Detector Z Offset from RP Detector Y Offset from RP
Changed:
<
<
0 4 (labeled in Figure 1) Phi -45deg, Theta 40deg (labeled in Figure 2) cm cm cm
1 1 (labeled in Figure 1) Phi -30deg, Theta 40deg (labeled in Figure 2) cm cm cm
2 2 (labeled in Figure 1) Phi -35deg, Theta 40deg (labeled in Figure 2) cm cm cm
3 3 (labeled in Figure 1) Phi -40deg, Theta 40deg (labeled in Figure 2) cm cm cm
>
>
0 4 (labeled in Figure 1) Phi -45deg, Theta 40deg Yellow (see Figure 2) cm cm cm
1 1 (labeled in Figure 1) Phi -30deg, Theta 40deg Red (see Figure 2) cm cm cm
2 2 (labeled in Figure 1) Phi -35deg, Theta 40deg Green (see Figure 2) cm cm cm
3 3 (labeled in Figure 1) Phi -40deg, Theta 40deg Blue (see Figure 2) cm cm cm
 

Figure 1

Please note that the original image is courtesy of the CCFE Drawing Office

Line: 26 to 26
 
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
Changed:
<
<
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
                   

>
>
20/08/13 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
08/19/13 29879     Werner Yes       Sawteeth

08/19/13 29879     Werner   Yes     Sawteeth  
08/19/13 29879     Werner     Yes   Sawteeth  
08/19/13 29879     Werner       Yes Sawteeth  
08/20/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29880     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29881     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/19/13 29882     Werner         Sawteeth  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/20/13 29920     Werner         Fishbone  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29958     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/21/13 29960     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29966     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
08/22/13 29972     Ramona         Beamblip  
 
                     
                     
                     
Deleted:
<
<
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
                     
 
                     
                     
                     

Revision 112014-01-29 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Detector Orientations

Changed:
<
<
Channel # Detector Position in Housing Angular orientation  
0 4 (in yellow in figure) Phi -45deg, Theta 40deg  
1 1 (in yellow in figure) Phi -30deg, Theta 40deg  
2 2 (in yellow in figure) Phi -35deg, Theta 40deg  
3 3 (in yellow in figure) Phi -40deg, Theta 40deg  
>
>
Channel # Detector Position in Housing Angular Orientation Orbit Trajectory Color Detector X (R) Offset from RP Detector Z Offset from RP Detector Y Offset from RP
0 4 (labeled in Figure 1) Phi -45deg, Theta 40deg (labeled in Figure 2) cm cm cm
1 1 (labeled in Figure 1) Phi -30deg, Theta 40deg (labeled in Figure 2) cm cm cm
2 2 (labeled in Figure 1) Phi -35deg, Theta 40deg (labeled in Figure 2) cm cm cm
3 3 (labeled in Figure 1) Phi -40deg, Theta 40deg (labeled in Figure 2) cm cm cm

Figure 1

  Please note that the original image is courtesy of the CCFE Drawing Office

detector_orientation_image.jpg

Added:
>
>

Figure 2

Graphical particle trajectory output from FEPP's modified Orbit Code

 

Data Log

Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes

Revision 102014-01-28 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

Back to MAST Diagnostic

Changed:
<
<

Detector Orientations

>
>

Detector Orientations

 
Channel # Detector Position in Housing Angular orientation  
0 4 (in yellow in figure) Phi -45deg, Theta 40deg  
1 1 (in yellow in figure) Phi -30deg, Theta 40deg  
2 2 (in yellow in figure) Phi -35deg, Theta 40deg  
3 3 (in yellow in figure) Phi -40deg, Theta 40deg  
Changed:
<
<
  • Click on below link to view image of Detector Positions in the PD Housing
  • detector_orientation_image_scaled.pdf
  • Please note that the original image is courtesy of the CCFE Drawing Office
>
>		Please note that the original image is courtesy of the CCFE Drawing Office
 
Changed:
<
<

Data Log

>
>		detector_orientation_image.jpg

Data Log

 
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
Line: 38 to 38
 
                     

META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"
Added:
>
>
META FILEATTACHMENT attachment="detector_orientation_image.jpg" attr="h" comment="" date="1390881395" name="detector_orientation_image.jpg" path="detector_orientation_image.jpg" size="207222" user="lc_2eramona" version="1"

Revision 92014-01-27 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Deleted:
<
<

Back to FEPP

 

Back to MAST Diagnostic

Added:
>
>

Detector Orientations

Channel # Detector Position in Housing Angular orientation  
0 4 (in yellow in figure) Phi -45deg, Theta 40deg  
1 1 (in yellow in figure) Phi -30deg, Theta 40deg  
2 2 (in yellow in figure) Phi -35deg, Theta 40deg  
3 3 (in yellow in figure) Phi -40deg, Theta 40deg  

  • Click on below link to view image of Detector Positions in the PD Housing
  • detector_orientation_image_scaled.pdf
  • Please note that the original image is courtesy of the CCFE Drawing Office

Data Log

 
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
Line: 25 to 36
 
                     
                     
                     
\ No newline at end of file
Added:
>
>
META FILEATTACHMENT attachment="detector_orientation_image_scaled.pdf" attr="h" comment="" date="1390857228" name="detector_orientation_image_scaled.pdf" path="detector_orientation_image_scaled.pdf" size="224975" user="lc_2eramona" version="1"

Revision 82014-01-22 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Line: 6 to 6
 

Back to MAST Diagnostic

Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Changed:
<
<
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
>
>
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is very noisy. Very few peaks have noisless bases.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
 
                   

                     
                     
                     
Changed:
<
<
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
>
>
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/analysis/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
 
                     
                     
                     

Revision 72014-01-15 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Line: 6 to 6
 

Back to MAST Diagnostic

Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
Changed:
<
<
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar Yes       Quiescent There was only noise after 0.3 seconds.
>
>
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar No       Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar Yes       Quiescent There was only noise after 0.3 seconds.
 
                   

                     
                     
                     
Changed:
<
<
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/082013Data/ Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
>
>
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/DataLog/QuiescentShots Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
 
                     
                     
                     

Revision 62014-01-09 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Added:
>
>

Back to FEPP

Back to MAST Diagnostic

 
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.

Revision 52013-12-11 - lc_2eramona

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Deleted:
<
<
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data
 		/data/plasma.1/Digitizer/082013Data/
 		Omar No Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar Yes Quiescent There was only noise after 0.3 seconds.


 
 
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/082013Data/ Omar Yes Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
 \ No newline at end of file
Added:
>
>
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No       Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No       Quiescent This channel is almost all noise.
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar Yes       Quiescent There was only noise after 0.3 seconds.
                   

                     
                     
                     
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/082013Data/ Omar   Yes     Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.
                     
                     
                     
                     
                     
                     
                     
                     
                     
 \ No newline at end of file

Revision 42013-12-07 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Line: 7 to 7
 
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data
 		/data/plasma.1/Digitizer/082013Data/
 		Omar No Quiescent This channel is almost all noise.
Changed:
<
<

>
>
20/08/2013 29906 ctrl_fim_29906_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar Yes Quiescent There was only noise after 0.3 seconds.
 


 

Revision 32013-12-07 - omaleo21

Line: 1 to 1
 
META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27
Changed:
<
<
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No       Quiescent This channel does not exhibit any charged particle peaks
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
                     
>
>
Shot Date Shot # Filename Directory Investigator - Date Ch0 Ch1 Ch2 Ch3 Scenario Notes
20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No Quiescent This channel does not exhibit any charged particle peaks
20/08/13 29907 ctrl_fm_29907_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29924 ctrl_fm_29924_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Omar No Quiescent This channel is almost all noise.
20/08/13 29929 ctrl_fm_29929_0.5_0.data
 		/data/plasma.1/Digitizer/082013Data/
 		Omar No Quiescent This channel is almost all noise.



 
 
20/08/13 29906 ctrl_fm_29906_0.5_1.data /data/plasma.1/Digitizer/082013Data/ Omar Yes Quiescent This channel had a possible overload at points .246 s to .256 s and .266 s to .296 s. There was only noise after 0.3 seconds.

Revision 22013-12-07 - Pavila

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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20/08/13 29908 ctrl_fm_29908_0.5_0.data /data/plasma.1/Digitizer/082013Data/ Pierre No       Quiescent This channel does not exhibit any charged particle peaks
 
                     
                     
                     

Revision 12013-11-27 - lc_2eramona

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META TOPICPARENT name="MAST_Diagnostic"
-- RamonaValenzuelaPerez - 2013-11-27

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