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Performance of the FOS Detectors in a Variable External Magnetic FieldWe present the results of an investigation of the in-orbit performance of the Digicon detectors in the Faint Object Spectrograph (FOS), conducted as part of the commissioning phase of the Hubble Space Telescope. This paper includes orbital results on detector background noise, sensor image stability, and photometric stability along with several typical FOS observations. New techniques for suppressing cosmic ray induced background and geomagnetic induced image motion in electron tube detectors are also discussed.
Document ID
19970016829
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Fitch, J. E.
(Space Telescope Science Inst. Baltimore, MD United States)
Hartig, G. F.
(Space Telescope Science Inst. Baltimore, MD United States)
Baity, W. A.
(California Univ., San Diego La Jolla, CA United States)
Beaver, E. A.
(California Univ., San Diego La Jolla, CA United States)
Cohen, R. D.
(California Univ., San Diego La Jolla, CA United States)
Junkkarinen, V. T.
(California Univ., San Diego La Jolla, CA United States)
Lyons, R. W.
(California Univ., San Diego La Jolla, CA United States)
Lindler, D. J.
(Advanced Computer Concepts, Inc. Potomac, MD United States)
Date Acquired
August 17, 2013
Publication Date
April 14, 1993
Publication Information
Publication: SPIE Proceedings Series
Publisher: Society of Photo-Optical Instrumentation Engineers
Volume: 1945
ISBN: 0-8194-1181-7
Subject Category
Astronomy
Report/Patent Number
NASA-CR-204023
NAS 1.26:204023
Meeting Information
Meeting: Space Astronomical Telescopes and Instruments 2
Location: Orlando, FL
Country: United States
Start Date: April 13, 1993
End Date: April 14, 1993
Accession Number
97N71535
Funding Number(s)
CONTRACT_GRANT: NAS5-24463
CONTRACT_GRANT: NAG5-1630
Distribution Limits
Public
Copyright
Public Use Permitted.
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