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Responsivity variations in the IRAS surveyThe IRAS survey detectors show nonlinear characteristics in their gains and baselines. This behavior can be described by an exponentially decaying gain enhancement, dependent on previously observed flux. The baseline behavior has been modeled by a decaying function composed of the sum of two exponential functions. The scale lengths are 10 arcmin and 1.1 deg for 12 microns, and 8 arcmin and 43 arcmin for 25 microns. Amplitude changes due to this type of hysteresis are less than 1 percent. In addition there is a considerable response of all detectors to particles associated with the South Atlantic Anomaly. Attempts to correct for this effect were performed on the 12- , 60- and 100-micron detectors in the form of bias boosts. This note presents a correction procedure for the 25-micron detectors.
Document ID
19900034639
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Deul, E. R.
(Leiden Rijksuniversiteit, Sterrewacht, Netherlands)
Walker, H. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 14, 2013
Publication Date
December 1, 1989
Publication Information
Publication: Astronomy and Astrophysics Supplement Series
Volume: 81
Issue: 2, De
ISSN: 0365-0138
Subject Category
Astronomy
Report/Patent Number
ISSN: 0365-0138
Accession Number
90A21694
Distribution Limits
Public
Copyright
Other

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