
Proceedings Paper
ISOPHOT: the imaging photopolarimeter for the Infrared Space ObservatoryFormat | Member Price | Non-Member Price |
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Paper Abstract
The flight model of ISOPHOT has been completed and delivered to ESA. The pre-flight calibration verified the high performance specifications for the far-infrared detector channels. At times, limiting factors in orbit may be high-energy-radiation induced noise and responsivity drifts after passage through the radiation belts, and signal drifts following large incident flux changes.
Paper Details
Date Published: 20 October 1993
PDF: 11 pages
Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); doi: 10.1117/12.158678
Published in SPIE Proceedings Vol. 1946:
Infrared Detectors and Instrumentation
Albert M. Fowler, Editor(s)
PDF: 11 pages
Proc. SPIE 1946, Infrared Detectors and Instrumentation, (20 October 1993); doi: 10.1117/12.158678
Show Author Affiliations
Dietrich Lemke, Max-Planck-Institut fuer Astronomie (Germany)
Juergen Wolf, Max-Planck-Institut fuer Astronomie (Germany)
Juergen Wolf, Max-Planck-Institut fuer Astronomie (Germany)
Josef Schubert, Max-Planck-Institut fuer Astronomie (Germany)
Michael A. Patrashin, Space Research Institute (Russia)
Michael A. Patrashin, Space Research Institute (Russia)
Published in SPIE Proceedings Vol. 1946:
Infrared Detectors and Instrumentation
Albert M. Fowler, Editor(s)
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