Modeling results are presented for proton-induced degradation of charge-coupled devices (CCDs) used in the Advanced CCD Imaging Spectrometer instrument on the Chandra X-Ray Observatory. A methodology is described that provides insights regarding degradation mechanisms and on-orbit performance for front-illuminated and back-illuminated CCDs. Proton-induced changes in charge transfer inefficiency are modeled. The observed amount of on-orbit degradation can be accounted for using a proton spectrum at the CCD location that has the same shape as the spectrum incident on the spacecraft but has a fluence that is reduced in magnitude by a factor of /spl sim/10/sup 5/.
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Lo et al. (2003) studied this question.
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