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17.4 Cosmic Rays
As with CCDs, cosmic ray hits will produce unwanted signal in the output images, but hot pixels are not expected to develop from such hits. Hence, cosmic rays should have little impact on the long-term array performance in orbit.
Analysis of SMOV data has shown that the rate of cosmic rays on the NICMOS detectors is about 1.2-1.6 events/Camera/sec (5
detections, see Instrument Science Report NIMOS-022). The mean size of the cosmic ray (CR) hits is 1.65 to 2 pixels. Table 17.2 below summarizes cosmic ray statistics for the three cameras, for 5
and 3
detections. The numbers for Camera 2 come from two different programs and indicate variations of about 60% in the rate of CR-affected pixels between the two observations; the variations reflect changes in the orbital position of the telescope relative to the South Atlantic Anomaly. This level of variation is what should be expected during a typical multi-orbit program.
CR Event Statistics
For a mean CR-affected pixel rate of about 2.5 pixels/sec, about 8% of the pixels in the detector will show cosmic ray events in a 2000 second exposure.
CR hits should be detected by calnica in MULTIACCUM data, and will be flagged in the DQ extensions of the *_ima.fits files.
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Last updated: 11/13/97 17:23:05