Asymptotically vanishing cosmological constant, Self-tuning and Dark Energy.
ECAL: HV tuning
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Transcript of ECAL: HV tuning
ECAL: HV tuning
Irina Machikhiliyan, 21.03.2012
• Input parameters:– π⁰ calibration latest (corresponds to the run #102323, 25 Sept
2011, provided by MN)– Outer border cells: PmPin ratios– Cells with changed Pm/C-W are excluded
• New HV test (5 TAE, 11 KHz ON):– run #108978 (10K) – old HV– run #108982 (10K) – new HV + LED intensity tuned
• MV consumption change (per side): 1.116A → 1.126A(No beam, no LED flashing)
ECAL HV adjustment test
Irina Machikhiliyan, 21.03.2012
K1 = required gain change
K1 / K2
I 25/41 ( k1 = 1.35)
K1 / K2
K1 – required gain change ( input parameter)K2 = PmToPin(new HV) / pmToPin(old HV) - measured gain change after HV adjustment
HV(new) / HV (old)
LED system time alignment (#108982)
Irina Machikhiliyan, 21.03.2012
P1 / (P1+T0+N1) P1 / (P1+T0+N1), averaged over LED
N1 / (P1+T0+N1), averaged over LEDN1 / (P1+T0+N1)
Timing is acceptable, but it would be better to make a tuning (after detector timing is checked with TAE events)
Further steps
Irina Machikhiliyan, 21.03.2012
• FEB fine delays check/tuning to account for new HV (m.p. done by Frederic)
• Calibration constants reset (m.p. done by Olivier)• Detector timing check with TAE• Final tuning of LED/PIN timing
Extra
Irina Machikhiliyan, 21.03.2012
PmPin change during the shutdown (1)
Irina Machikhiliyan, 21.03.2012
Reference runs: #104406 (beginning of the fill 2267, 30 Oct 2011)# 108978 (12 Mar 2012)
PmPin(12 Mar)/PmPin(30 Oct)
PmPin change during the shutdown (2)
Irina Machikhiliyan, 21.03.2012
PmPin(12 Mar)/PmPin(30 Oct), Inner
PmPin(12 Mar)/PmPin(30 Oct), Middle
PmPin(12 Mar)/PmPin(30 Oct), Outer
Average recovery is on the level of 8÷13%, strongly depends on the detector area (up to 25% in the “horns”)