Detector 2 anneal 2012

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Detector 2 has been unsegmented since the 2012 anneal. The entire detector volume is read out through the front segment electronics, so rates look higher for G2 (and also G4) than for the other detectors.

Detector 2 is located in a position where it can receive light leak through a valve at the back of the cryostat. This problem occurs when the back of the spacecraft is pointed towards the sunlit earth, so it comes and goes with the orbital precession. Light leak only affects the rear sections of the detector, but since Detector 2 is unsegmented, the excess counts are seen in the front segment readout. Symptoms of this problem are enhanced reset rates and fast LLD rates, and the problem does degrade livetime. (Example) Raising the LLD level can ease the livetime problem, but this will have a negative effect on lower-energy spectroscopy. Light leak can be seen to a lesser extent in detector 3, and very rarely in 5 and 9.

2012 March 30 17:53:27 UT: The front fast event threshold for detector 2 was raised by 0x10, from 0x60 to 0x70, to free up livetime (due to light leak problem)

2012 August 1: In the past week detector 2 livetime has occasionally been compromised by the light leak problem. No action is being taken, since we do not want to impair low-energy spectroscopy.

2012 November 6: There was a bit of noise on detector 2, so the front slow threshold was raised from 0x60 to 0x78. This may help with the SSR fill level issues we have been seeing recently.

2013 January 24: The high voltage of detector 2 was raised by five steps (211 -> 216). The voltage is now at 4215V.

2013 January 30: The high voltage of detector 2 was raised by five steps (216 -> 221).

2013 February 5: The detector 2 high voltage was raised by another five steps (221 -> 226). This increase puts G2 at 4411 V, which is now the highest voltage of all our detectors.