MUST2 SAMURAI_2018 S3-LEB-LPC SUPERNEMO MUGAST EXPAND SCALP GALATRON HiCARI VELO
  MUGAST, Page 3 of 132  Not logged in MUGAST
New entries since:Thu Jan 1 01:00:00 1970
Status ExpNbr Date Author Type Category Target-Source Subject
FixedTEST Tue Mar 5 18:03:24 2019 iulian MarleneMUST2SoftwareN/ACalimero problem on Y side
Calimero not working properly on Y side of any mm detector
Attachment 1: run83_calimero_mm4Y_spectra.png
run83_calimero_mm4Y_spectra.png
Attachment 2: run834calimero_mm2Y_spectra.png
run834calimero_mm2Y_spectra.png
FixedTEST Tue Mar 5 18:18:46 2019 iulian MarleneMUST2Hardware3-alpharun 97 3a run Muvi3 night run
Run 87

stop@ 5:42 am

3a run Muvi3 (MM)
-4 deg
pedestals aligned and suppressed
Attachment 1: run87_3alpha_4mm_spectra.png
run87_3alpha_4mm_spectra.png
FixedTEST Wed Mar 6 15:02:51 2019 ValerianMUST2Hardware3-alphaCooling temperature is relevant for the resolution
Using run 52 -> 13deg and run 87 -> -5deg.

We see that the resolution improves at -5 degree. See attached picture as an example for MM2 X.
Attachment 1: MM2X_13deg.png
MM2X_13deg.png
Attachment 2: MM2X_minus5deg.png
MM2X_minus5deg.png
FixedTEST Thu Mar 7 09:29:47 2019 MarleneGRITGeneral run 96 double alpha source run shifted 60mm
RUN 96

double alpha source
MG1
MG3
MG4
MG5

MG7
-
-
MG11

MM1
MM2
MM3
MM4

Missing strips in Y the same as in run 40

Problem with the annular MG11 -> no current when bias is put... --> to be checked

Problem with the insertion of the target holder --> solved

I also checked again MG9 (still noisy)
and MG10 with 140V I=0,52uA and counting rate is the same order of magnitude as trapezoid. Spectra are OK (not saved).
Attachment 1: run96_MG7_MG11notworking.png
run96_MG7_MG11notworking.png
Attachment 2: run96_3alphasource_shifted_MG1-5.png
run96_3alphasource_shifted_MG1-5.png
Attachment 3: run96_HV2.png
run96_HV2.png
Attachment 4: run96_HV1.png
run96_HV1.png
FixedTEST Thu Mar 7 14:02:03 2019 Marlène IulianMUST2GeneralN/Atest of MUST2 electronics
Test with pulser at 20 kHz
The OR of MUVI was scaled down by a factor of 100, to provoke some resets
Fixed  Tue Mar 12 10:21:17 2019 MarlèneMUST2General Debug Calimero Y
Debug of Calimero

test of channels (mate) masking : OK with DAS, OK with GECCO (see attachment) when done in the "disable channels" of GECCO

With calimero, when we are on Y, when we click right to mask a mate we see 'disable mate 2' instead of 'disable mate 10' !!!
Attachment 1: test_GECO_masquage_mate2&10activees_seulement.png
test_GECO_masquage_mate2&10activees_seulement.png
FixedTEST Mon Mar 18 18:31:18 2019 valerian marlèneGRITGeneral3-alphaRUN 20 (com2019) 3 alpha overnight
RUN20

Run with double 3alpha source MUST2+MG1_7+MG11
temperature -4 deg on both cooling

Acquisition with VAMOS+MUGAST coupled (com2019)

Time range =600ns
pedestal aligned and suppressed

run start at 18h23 monday 18

run stop at 8h34 tuesday 19

about 12Go of data
Attachment 1: RUN20_HV_MG_3lapha.png
RUN20_HV_MG_3lapha.png
Attachment 2: RUN20_3alpha_HV_MUST2.png
RUN20_3alpha_HV_MUST2.png
Fixed  Tue Mar 19 19:35:53 2019 marleneGRITGeneral RUN 98 3alpha source all detectors
RUN 98
3 alpha source
all detectors (trap,square, MUST2,annular)
Temp=15deg
Acquisition mugast
FixedTEST Thu Mar 21 10:37:47 2019 Adrien and ValerianMUST2GeneralN/ATest TOF must2
To make sure the mate work correctly we took an alpha run with a delayed fag on the MUVI stop:
- all mate register a time in the the middle of the range as expected (fag delayed by 350ns, range is 600ns)

Test with time calibrator, all channel are enable, pulser on channel 3 of each mate T1X:
- energy spectrum: pulser where we expect it.
- we expect to see a time calibrator spectrum on channel 3 of each mate. instead we see times spectrum on Channel 3 of mate 1 and 2, channel 12 of mate 1, channel 14 of mate2. nothing else

Conclusion

The problem was that the synctst had to be checked and ord unchecked
Attachment 1: Time_behavior_withDAS.png
Time_behavior_withDAS.png
FixedTEST Thu Mar 21 13:28:06 2019 Valerian and AdrienDAQSoftwareN/AFirst fully functionnal time calibration run on X and Y of MG1
Our program is able to perform the time calibration of our detector for both X and Y, see picture attached.
Attachment 1: CALIMEROY1.png
CALIMEROY1.png
Attachment 2: FIRST_TIMECALIBRATION_WITHOUT_CALIMERO.png
FIRST_TIMECALIBRATION_WITHOUT_CALIMERO.png
FixedTEST Fri Mar 22 17:28:09 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 117
- MUVI: MUVI1
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
FixedTEST Fri Mar 22 17:37:37 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 118
- MUVI: MUVI1
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
FixedTEST Fri Mar 22 17:47:04 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 119
- MUVI: MUVI2
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
FixedTEST Fri Mar 22 17:56:37 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 120
- MUVI: MUVI2
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
FixedTEST Fri Mar 22 18:06:11 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 121
- MUVI: MUVI3
- Side : MUFEE X (Junction)
- Telescope: 1, 2, 3, 4
FixedTEST Fri Mar 22 18:15:39 2019 OttoRUNGeneralN/ATimeCalibratorRun
*** Run Time Calibrator FSC ***
- Run: 122
- MUVI: MUVI3
- Side : MUFEE Y (Ohmic)
- Telescope: 1, 2, 3, 4
FixedTEST Sat Mar 23 15:26:06 2019 Adrien MattaOTHERSoftwareN/ATo do list
FSC:

  • Autoconf programme to set all regular parameter (PAC gain, TAC range, ORD, no mask, no pulser)


Sentinel:
  • Making the program
  • Preparing start script
  • Preparing stop script
  • Preparing init script


Online/offline:
  • Look into ZMQ to replace GRU
  • Datum through zmq
  • Switch NPSpectraServer/Client to ZMQ and datum
  • CsI Calibration with db scan
  • 3-alpha calibration using NPCalibration

HV:
  • Remote read
  • Auto logging
  • Alert on trip
  • Bt/HV/sector on/off
FixedTEST Wed Mar 27 11:06:33 2019 Valerian and CyrilGRITHardware3-alphaEvolution of resolution with temperature
For the mugast telescope, changing the temperature from 13deg to minus 4deg doesn't seem to have an impact as strong as for the MUST2 telescopes.
Still, the resolution improve with a lower temperature, but the improvement is of only 0.1 channel... (See joined screenshots)
Attachment 1: MG4_13_deg.png
MG4_13_deg.png
Attachment 2: MG4_minus_4_deg.png
MG4_minus_4_deg.png
FixedTEST Thu Mar 28 14:22:25 2019 OttoRunRUNGeneralN/ATEST
Run : 146
Date : 28/03/2019

Start: 14:22:25
asdasdasdasd

Stop: 14:22:42
asdasdasdasd
FixedTEST Thu Mar 28 15:39:01 2019 ValerianOFFLINESoftwareN/AStatus of the converion with VAMOS program
The conversion with VAMOS program was validated using run_0020 from com2019


Program output as a ref :

T1 : 9978458
T2 : 9978458
checking multiplicities
Reading: 99.9152 %MULTIPLICITIES OK!
checking values
Reading: 99.9152 %%
DETECTOR NUMBERS ARE OK!!!!!
STRIP NUMBERS ARE OK!!!!!
ENERGY VALUES ARE OK!!!!!
TIME VALUES ARE OK!!!!!

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