AIDA
GELINA
BRIKEN
nToF
CRIB
ISOLDE
CIRCE
nTOFCapture
DESPEC
DTAS
EDI_PSA
179Ta
CARME
StellarModelling
DCF
K40
AIDA
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Entry time:
Sat Mar 29 12:37:19 2025
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*2:30 pm*: changed power source of USB-controlled power supply for FEEs. Now one of the power cables is connected to the 'B' power supply of F11, and the second to the 'C' power supply (these are in the unit on top of WASBI crates). The reason for change is that before both were connected to 'C', and drained current was very close to limit of 10 A (and power cord getting noticeable hot). We'll check resolution after this switch. Detectors 1, 2, 3, and 4 biased to 100V, detectors 5, 6, and veto biased to 70V. n-side is more noisy than p-side, but resolution comparable to previous configuration: NNAIDA# FWHM [ch] 1 91 2 61 3 84 4 - 5 160 6 - 7 79 8 84 9 71 10 76 11 101 12 81 13 69 14 78 15 199 16 107 17 82 18 62 19 - 20 89 21 168 22 70 23 80 24 73 25 81 26 13 27 109 28 13 29 15 30 126 31 13 32 100 *5 pm*: Set-up correlation scalers for AIDA<->EURICA<->BigRIPS (detail diagram coming soon, now only in paper logbook). *6:30 pm*: Started EURICA DAQ with Pieter and Gabor. A folder is created to record data of June campaign: /raid/11/mbs/2016_ucampaign/ Tested correlation of AIDA and EURICA with a pulser run, triggering EURICA and AIDA correlation scaler with 250 Hz. The corresponding files are /raid/11/mbs/2016_ucampaign/test0003.lmd /TapeData/may2016/R12_0.gz Phong did a quick analysis and the pattern of correlation scalers in both files is similar (attached figures). It is also consistent with the number of reset requests we sent during the data taking (three requests closely spaced in the middle of run, and two more in the end of the run).
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