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Proceedings Paper

Linear polarization sensitivity specifications for spaceborne instruments
Author(s): Peter William Maymon; Russell A. Chipman
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Paper Abstract

The radiometric accuracy of space-borne instruments such as radiometers and spectroradiometers which make measurements of the earth and other celestial objects can be compromised by the linear polarization sensitivity (LPS) induced by the optical system. Most of these optical systems contain optical elements whose reflectance or transmission is polarization dependent, such as diffraction gratings, folding and scanning mirrors, dichroic filters, and optical fibers. Optical system incorporating such elements generally display linear polarization sensitivity; different linear polarization states incident with equal radiometric power will be measured as different power levels. If the incident polarization state is unknown, the linear polarization sensitivity cannot be compensated during the data reduction. The light reflected from the earth and other planets and moons is usually partially linearly polarized, but in a random distribution. Thus, to make accurate radiometric measurements of these bodies, a radiometer or spectrometer should have a low level of linear polarization sensitivity. This paper contains a mathematical description of LPS, contains references to systems which have imposed a LPS specification, describes some of the sources of LPS, describes how to model LPS by polarization ray tracing, and discusses methods to reduce the LPS of an optical system.

Paper Details

Date Published: 11 December 1992
PDF: 9 pages
Proc. SPIE 1746, Polarization Analysis and Measurement, (11 December 1992); doi: 10.1117/12.138783
Show Author Affiliations
Peter William Maymon, NASA Goddard Space Flight Ctr. (United States)
Russell A. Chipman, Univ. of Alabama in Huntsville (United States)


Published in SPIE Proceedings Vol. 1746:
Polarization Analysis and Measurement
Dennis H. Goldstein; Russell A. Chipman, Editor(s)

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