Design of precise ultraviolet imaging polarimeters that rely on in situ calibration

Details Design of precise ultraviolet imaging polarimeters that rely on in situ calibration Design of precise ultraviolet imaging polarimeters that rely on in situ calibration

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994spie.2010..192n&link_type=abstract

Proc. SPIE Vol. 2010, p. 192-200, X-Ray and Ultraviolet Polarimetry, Silvano Fineschi; Ed.

Computer Science

Scientific paper

A telescope design based upon oblique reflections can give an efficient UV, EUV, or X-ray imaging complete-Stokes polarimeter. Oblique reflections from mirror surfaces can be efficient giving both retardation and polarization-analyzing effects. In situ methods using a linearly polarized source can determine the Jones matrix for the optical system uniquely. Rotation of the purely polarized source provides a direct method for calibrating any nondepolarizing optical system to high accuracy.

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