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Measurements with the Chandra X-ray Observatory's Flight Contamination MonitorNASA's Chandra X-ray Observatory includes a Flight Contamination Monitor (FCM), a system of 16 radioactive calibration sources mounted to the inside of the Observatory's forward contamination cover. The purpose of the FCM is to verify the ground-to-orbit transfer of the Chandra flux scale, through comparison of data acquired during the ground calibration with those obtained in orbit, immediately prior to opening the Observatory's sun-shade door. Here we report results of these measurements., which place limits on the change in the mirror-detector system response and, hence, on any accumulation of molecular contamination on the mirrors' iridium-coated surfaces between the two sets of measurements.
Document ID
20110000859
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Elsner, R. F.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Kolodziejczak, J. J.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
ODell, S. L.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Swartz, D. A.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Tennant, A. F.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Weisskopf, M. C.
(NASA Marshall Space Flight Center Huntsville, AL, United States)
Date Acquired
August 25, 2013
Publication Date
March 27, 2000
Subject Category
Optics
Meeting Information
Meeting: Measurements with the Chandra X-ray Observatory''s Flight Contamination Monitor
Location: Munich
Country: Germany
Start Date: March 27, 2000
End Date: March 31, 2000
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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