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Using ACIS on the Chandra X-ray Observatory as a Particle Radiation Monitor IIThe Advanced CCD Imaging Spectrometer is an instrument on the Chandra X-ray Observatory. CCDs are vulnerable to radiation damage, particularly by soft protons in the radiation belts and solar storms. The Chandra team has implemented procedures to protect ACIS during high-radiation events including autonomous protection triggered by an on-board radiation monitor. Elevated temperatures have reduced the effectiveness of the on-board monitor. The ACIS team has developed an algorithm which uses data from the CCDs themselves to detect periods of high radiation and a flight software patch to apply this algorithm is currently active on-board the instrument. In this paper, we explore the ACIS response to particle radiation through comparisons to a number of external measures of the radiation environment. We hope to better understand the efficiency of the algorithm as a function of the flux and spectrum of the particles and the time-profile of the radiation event.
Document ID
20120015357
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Grant, C. E.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Ford, P. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Bautz, M. W.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
ODell, S. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 26, 2013
Publication Date
July 1, 2012
Publication Information
Publication: Proceedings of SPIE
Volume: 8443
Subject Category
Instrumentation And Photography
Report/Patent Number
M12-1930
Meeting Information
Meeting: Space Telescopes and Instrumentation 2012: Ultraviolet to Gamma Ray
Location: Amsterdam
Country: Netherlands
Start Date: July 1, 2012
End Date: July 6, 2012
Sponsors: International Society for Optical Engineering
Funding Number(s)
CONTRACT_GRANT: NAS8-38252
CONTRACT_GRANT: NAS8-37716
Distribution Limits
Public
Copyright
Public Use Permitted.
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