Telescopic polarimetry of planetary bodies - An overview

Details Telescopic polarimetry of planetary bodies - An overview Telescopic polarimetry of planetary bodies - An overview

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1747..253d&link_type=abstract

In: Polarization and remote sensing; Proceedings of the Meeting, San Diego, CA, July 22, 23, 1992 (A93-30026 11-35), p. 253-261.

Physics

Light Scattering, Linear Polarization, Planets, Polarimetry, Space Observations (From Earth), Surface Roughness, Interplanetary Dust, Mars Surface, Moon, Planetary Atmospheres, Soils, Telescopes

Scientific paper

Developments in theoretical and experimental research of planetary bodies based on telescopic polarimetry are reviewed. Topics discussed include different polarimetric techniques based on visual fringe, photoelectric, and CCD video polarimeters; optical polarimetry on solar system objects; polarization of rough surfaces; soil physics on planetary surfaces; the surface of Mars; cometary physics and dust grains; and mists, clouds, and storms in Venus, Jupiter, Saturn, and Mars atmospheres.

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