nextuppreviouscontents
Next:The MIT Model of Up:ACIS CCD Sensitivity to Previous:Effects of Energetic Protons

Search for Effects of Short Exposure to Low-Earth Orbit on ACIS CCD Peformance

Two calibrated ACIS CCID17 units were flown aboard Space Shuttle Discovery for a 12 day mission in August 1997. (STS 85, OV-103) The devices, w157c1 and w147c3 (back illuminated) were in the normal input-shorted storage configuration in the standard shipping container which was stowed in the pressurized crew compartment.

Testing immediately before and after flight showed no change in performance for either device. Neither an increase in the number of hot or flickering pixels nor any CTI increase due to radiation exposure was seen.

Pre- and post-flight mean dark current maps for the two test devices are compared in figures 4.122 and 4.123. These images are averages of at least ten individual exposures, each of 18 seconds. All except the pre-flight image of w157c1 (the front-illuminated device) were obtained with the detector temperature at -120C; the preflight image of w157c1 was obtained at -60C. The front illuminated device w157c1, which had a small edge glow and a bright defect prior to flight, showed no evidence of either feature during any post-flight testing. This change may have been a consequence of handling and may have nothing to do with the shuttle orbital environment. We conclude that low earth orbit shuttle cabin environment has no impact upon CCD performance for 1 week exposures.
 
 

Figure 4.122: Dark current for the front-illuminated device w157c1 before (top) and after (bottom) its flight on STS-85. The preflight image was obtained at -60 C and the postflight image at -120C. The bright defect was invisible at any temperature after the shuttle flight. The images are shown with identical colors scales; the signal level, in electrons per pixel per 18 s, is shown. Quadrant C was defective before and after the flight.
 
 

Figure 1.123: Dark current for the back-illuminated device w147c3 before (top) and after (bottom) its flight on STS-85. There is no apparent increase in the dark current. Both images were obtained at -120C. The same color scale is used for the two images; the signal level, in electrons per pixel per 18 s, is shown on the color bar.


nextuppreviouscontents
Next:The MIT Model of Up:ACIS CCD Sensitivity to Previous:Effects of Energetic Protons
Please address comments and questions to Dr. John Nousek ( nousek@astro.psu.edu )