| Status |
ExpNbr |
Date |
Author |
Type |
Category |
Target-Source |
Subject |
| Fixed | TEST |
Fri Dec 14 09:08:46 2018 |
Adrien Matta | OTHER | Social | N/A | Test Post |
| MUGAST ELOG is now ONLINE |
| Fixed | TEST |
Wed Jan 16 16:33:28 2019 |
Marlène | GRIT | General | 3-alpha | Status of detectors on 16/01/19 |
| MG1 has some issue with the HT cable (for the BT bias). There is a shortcut only under vacuum. We checked the connector but we have to do vacuum again to check it. |
| Attachment 1: Detectors_status_160119.xlsx
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| Attachment 2: Capture_d’eÌcran_2019-01-16_aÌ€_17.05.57.png
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| Fixed | TEST |
Wed Jan 16 17:36:30 2019 |
Valérian-Marlène | GRIT | General | N/A | Calimero tests - How to configure Calimero in GECO |
Tests of Calimero time calibration with MUVI1 channel 2 (MM2)
1- channel 3 of all mates selected (see screeshots)
2- channel 1 of all mates
3- channel 1 of all mates - with channels enabled !!!!!
4- channel 1 of all mates - with channels enabled !!!!!
5- all channels telescope MM2
Number of counts = total number of counts for one channel on all mates
Conclusion :
Options to be chosen
1- with channels enabled
2- 10000 for the statistics
Remarks
To run calimero on MUVI1, caliWatcher should be set to 10202 and CaliSlave to 10223
The opposite for MUVI2, caliWatcher 10223, CaliSlave 10202 |
| Attachment 1: Calimero_MUVI1_MM2_voie3_allmates_bidim.png
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| Attachment 2: Calimero_MUVI1_MM2_voie1_allmates_bidim.png
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| Attachment 3: Calimero_MUVI1_MM3_voie1_allmates_bidim_withchannelsenabled.png
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| Attachment 4: Calimero_MUVI1_MM3_voie3_allmates_bidim_withchannelsenabled.png
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| Attachment 5: Calimero_MUVI1_MM2_allchannels_allmates_bidim_stat100000_withchannelsenabled.png
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| Fixed | TEST |
Fri Jan 18 15:32:50 2019 |
Adrien Valérian | GRIT | General | N/A | Calimero tests Muvi2 MM7 MG10C |
After disabling nptool Multithreading, online is working fine again.
Concerning Calimero, it is currently working both on MUVI1 and MUVI2 for the X at least.
Joined here is the result of Calimero for MG10C on MUVI2 channel 3 (MM7). |
| Attachment 1: Calimero_MUVI2_MM7_allchannels_allmates__stat100000_withchannelsenabled.png
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| Attachment 2: Calimero_MUVI2_MM7_allchannels_allmates_withchannelsenabled.png
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| Fixed | |
Tue Jan 22 11:15:15 2019 |
Marlène | GRIT | General | N/A | Square detectors |
MG9C (thin square detector coupled with thick square detector unplugged) noisy
On X channels --> no noise problem ( about 100 ORD in the dark)
On Y channels --> MATE 10 & 11 noisy ! (see picture below with noisy Y piedestals)
With internal pulser (trigered by CK_TST) the counting rate is OK only if the thresholds are set at 1 MeV. If they are set at 500 keV, the counting rate is 10 times higher than the CK_TST
For MG10C, ORD is OK ! |
| Attachment 1: MG9C_disabled_channels__no_crazy_ORD.png
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| Attachment 2: MG9C_disabled_channels__no_crazy_ORD_moredetailed.png
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| Attachment 3: MG9C_piedestal_of_disabled_channels_Y.png
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| Ongoing | TEST |
Tue Jan 22 18:52:23 2019 |
Valérian-Marlène | GRIT | General | 3-alpha | 3 alpha source run on MG10C & MG3T |
3 alpha source (not centered)
MG10C and MG3T ON
MG10C is connected to MG5T HT and BT and seen on MUVI1 channel2 -> online name=MM2
MG3T is connected to MG3T HT and BT and seen on MUVI1 channel3 -> online name=MM3
Attached : current and bias of the detectors |
| Fixed | TEST |
Wed Jan 23 09:11:26 2019 |
Valérian-Marlène | GRIT | General | 3-alpha | RUN9 : 3 alpha source run on MG10C & MG3T |
RUN 9 (over night 22/01 ->23/01)
3 alpha source (not centered)
MG10C and MG3T ON
MG10C is connected to MG5T HT and BT and seen on MUVI1 channel2 -> online name=MM2
MG3T is connected to MG3T HT and BT and seen on MUVI1 channel3 -> online name=MM3
Attached : current and bias of the detectors (decreasing with time)
+ online spectra for 3 alpha source run
MG10C has 7 missing strips ! (see attached spectrum) |
| Attachment 1: 3alpha_sourceMG10C-MM2_MG3T-MM3.png
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| Attachment 2: HV_squares_plugged_on_MG4T-MG5T_andMG3T.png
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| Attachment 3: HV_squares_plugged_on_MG4T-MG5T_andMG3T_afternightrun.png
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| Attachment 4: MG10C_7missingstrips.png
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| Fixed | |
Wed Jan 23 12:24:10 2019 |
Marlène | GRIT | General | | Change cable MG1T - Exchange of detectors named MG9C & MG10C |
23/01/19
Change of the HT/BT cable of MG1T (the one that had a short cut before when the chamber was closed)
MG9C is now the square detector nb 4 (Micron number) and coupled with the thick detector --> this detector was working properly
MG10C is detector nb 3 (Micron number) --> this detector was noisy before |
| Fixed | |
Fri Jan 25 17:02:25 2019 |
Marlène | GRIT | General | | Detectors numbering |
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| Attachment 1: MUGAST_detectors.pdf
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| Fixed | TEST |
Thu Feb 7 09:52:08 2019 |
Freddy, Marlène | RUN | General | 3-alpha | RUN10 : 3 alpha source on MG1-3-4-5-7 |
Test run with alpha source in front of trapezoid detectors.
First run with new LABELS updated from "MM" to "MG0" in GECO.
name : run_0010.dat.06-02-19_19h08m11s (1.4 GB)
date: 06/02/2019
start: 19:08
stop: ~22:00 |
| Attachment 1: alpha_source_5trap_rawhistos_2.png
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| Attachment 2: alpha_source_5trap_rawhistos.png
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| Fixed | |
Thu Feb 14 08:50:58 2019 |
Marlene | GRIT | General | 3-alpha | RUN 27 |
RUN 27 on 14th of feb.
3 alpha source (one in front of trap., one in front of square detectors)
MG10, MG4, MG7 and MG5 are OK.
MG1 shows alpha but at lower energy and with bad resolution (particularly on X). We suspect it is not well depleted. We tried to increase the bias up to 200V but did not see any change.
It is due to a non working SA/SL external cable that produces this error (we tested it with several detectors, we also tried to change the MUVI channel and it still does the same)
Conclusion :
We have tested all trapezoid detectors (MG1, MG3, MG4, MG5, MG7) the annular (MG11) and the thin square (MG10) they are all OK
Detectors (order in the GMT) :
MG10
MG1
MG4
-
MG7
MG5
-
-
attached : bias of detectors ( be careful : MG10 bias = MG11A)
spectra for all detectors |
| Attachment 1: HV_detectors_MG10_MG1_MG4_MG7_MG5.png
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| Attachment 2: GMT8config_HV_detectors_MG10_MG1_MG4_MG7_MG5.png
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| Attachment 3: 3alpha_sourceMG07X.png
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| Attachment 4: 3alpha_sourceMG07Y.png
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| Attachment 5: 3alpha_sourceMG05XY.png
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| Attachment 6: 3alpha_sourceMG10XY.png
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| Attachment 7: 3alpha_sourceMG04XY.png
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| Attachment 8: 3alpha_sourceMG01XY.png
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| Fixed | |
Thu Feb 14 15:30:14 2019 |
Marlene Daniele Jenny | GRIT | General | 3-alpha | RUN 28 |
RUN 28 14th Feb
3 alpha source on MG11A, MG3T, MG1T
GMT channels
MG11
-
MG3
-
-
MG1
- |
| Attachment 1: 3alpha_sourceMG03XY._OKpng
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| Attachment 2: 3alpha_sourceMG11XY.png
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| Attachment 3: 3alpha_sourceMG01XY_OK.png
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| Fixed | |
Fri Feb 15 15:31:28 2019 |
Marlène | GRIT | General | N/A | Detectors bias |
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| Fixed | com2019 |
Mon Feb 18 10:41:36 2019 |
Marlene | GRIT | General | N/A | Bias & current of detectors |
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| Attachment 1: bias.png
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| Fixed | TEST |
Thu Feb 21 09:08:49 2019 |
Freddy | RUN | General | 3-alpha | RUN 30 - alpha on MG 1,3,5,7 |
Run 30
Alpha source run for trapezoid detectors during the night with pedestals aligned and zero suppression. Cooling at 15°C.
Thresholds at 500 keV.
Run size: 1.3 G
On MUVI1:
1--> MG5 (150V)
2--> --
3--> MG3 (160V)
4--> --
On MUVI2:
5--> MG7 (120V)
6--> MG1 (140V)
7--> --
8--> --
TRIGGERS are:
GMT ch1 --> OR MUVI1
GMT ch2 --> OR MUVI2
GMT ch3 --> OR MUVI3 (nothing on it)
Plots are now represented using the correspondance map which means that it correspond to the geometrical ordering on the detector. With this representation groups of strips missing or disfunctionning on a given region of the detector is more obvious. |
| Attachment 1: 3alpha_source_MG_1357_20Feb.png
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| Attachment 2: LowV_bis_run30.png
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| Attachment 3: LowV_run30.png
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| Attachment 4: HV_run30.png
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| Fixed | TEST |
Thu Feb 21 14:37:26 2019 |
iulian, valerian &Freddy | GRIT | Hardware | 3-alpha | Results Calibration 3-alpha RUN30 MG1, MG3,MG5 & MG7 |
Results of the calibration run 30
In order:
Telescope1 X,Y (MG5 X,Y)
Telescope4 X,Y (MG3 X,Y)
Telescope7 X,Y (MG7 X,Y)
Telescope9 X,Y (MG1 X,Y) |
| Attachment 1: Telescope1Summary.pdf
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| Attachment 2: Telescope1Summary.pdf
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| Attachment 3: Telescope4Summary.pdf
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| Attachment 4: Telescope4Summary.pdf
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| Attachment 5: Telescope7Summary.pdf
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| Attachment 6: Telescope7Summary.pdf
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| Attachment 7: Telescope9Summary.pdf
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| Attachment 8: Telescope9Summary.pdf
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| Fixed | TEST |
Thu Feb 21 16:43:45 2019 |
Valérian, Freddy, Iulian and Marlène | GRIT | Hardware | N/A | Current measurements |
Joined are the the I(V).
Detectors seems to respond accordingly with the previous measurements from Marlène.
Annular detector curve is quite strange…
Joined files :
Depletion_Mugast_MG.pdf -> summary for trapezoidal + annular detectors
Depletion_Mugast_M2.pdf -> summary for Must2 detectors
Depletion_Mugast.xlsx -> Excel file |
| Attachment 1: Depletion_Mugast_MG.pdf
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| Attachment 2: Depletion_Mugast_M2.pdf
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| Attachment 3: Depletion_Mugast.xlsx
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| Fixed | TEST |
Thu Feb 21 17:32:42 2019 |
iulian, freddy | GRIT | Hardware | 3-alpha | run 33 3 alfa with MG1,MG3,MG4,MG5,MG7,MG9 short run |
First test of the repaired 2xcables. The repaired cables were placed between MUVI1_2 <=> MG4 & MUVI1_4 <=>MG11 (longer cable)
Correspondance for the rest is the same as for run 30. The mapping is the same for all detectors (including anulaire detector).
Alpha source run for trapezoid detectors + anulaire detector with pedestals aligned and zero suppression. Cooling at 15°C.
Thresholds at 500 keV.
On MUVI1:
1--> MG5 (150V)
2--> MG4 (95V)
3--> MG3 (160V)
4--> MG11 (60V)
On MUVI2:
5--> MG7 (120V)
6--> MG1 (140V)
7--> --
8--> --
TRIGGERS are:
GMT ch1 --> OR MUVI1
GMT ch2 --> OR MUVI2
GMT ch3 --> OR MUVI3 (nothing on it) |
| Attachment 1: 3alpha_sourceMG1MG4MG7MG9XY_run33.png
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| Attachment 2: 3alpha_sourceMG3MG5XY_run33.png
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| Fixed | TEST |
Thu Feb 21 18:14:48 2019 |
iulian | GRIT | Hardware | 3-alpha | ACQ problem run 34 3 alfa with MG1,MG3,MG4,MG5,MG7,MG9 |
Alpha source run for trapezoid detectors + anulaire detector with pedestals aligned (with HV  ) and zero suppression. Cooling at 15°C.
Thresholds at 500 keV.
On MUVI1:
1--> MG5 (150V)
2--> MG4 (95V)
3--> MG3 (160V)
4--> MG11 (60V)
On MUVI2:
5--> MG7 (120V)
6--> MG1 (140V)
7--> --
8--> --
TRIGGERS are:
GMT ch1 --> OR MUVI1
GMT ch2 --> OR MUVI2
GMT ch3 --> OR MUVI3 (nothing on it)
PROBLEM ACQ , MUVI2 has no validations (DECS). MUVI1 OK!. Looks like a problem on the catchslave actor of Narval as no events seems to pass trough
The problem was caused by the cable used to triger the GMTSlave from the FanIn FanOut. |
| Attachment 1: acq_problem_21and22fevrier.png
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| Fixed | TEST |
Fri Feb 22 11:56:53 2019 |
iulian | GRIT | Hardware | 3-alpha | run 38 3-alpha with reordering of the MUGAST cables for the logic and analogic signals |
Run 38
Alpha source run for trapezoid detectors during the night with pedestals aligned (with HV on) and zero suppression. Cooling at 15°C.
Thresholds at 500 keV.
Important:
The MUGAST signal cables (logic & analogic) have been reordered:
On MUVI1
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Channel | Spectra Label | Detector | Voltage
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1 | MG1 | MG1 | 140V
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2 | MG3 | MG3 | 160V
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3 | MG4 | MG4 | 95V
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4 | MG5 | MG5 | 150V
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On MUVI2:
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Channel | Spectra Label | Detector | Voltage
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1 | MG7 | MG7 | 120V
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2 | MG9 | MG11 | 60V
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3 | MG10 | -- | --
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4 | MG11 | -- | --
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TRIGGERS are:
GMT ch1 --> OR MUVI1
GMT ch2 --> OR MUVI2
GMT ch3 --> OR MUVI3 (nothing on it) |
| Attachment 1: run38_3alpha_mg1345.png
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| Attachment 2: run38_3alpha_mg711.png
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