Infrared Optical Constants of Martian Dust Derived from Martian Spectra

Details Infrared Optical Constants of Martian Dust Derived from Martian Spectra Infrared Optical Constants of Martian Dust Derived from Martian Spectra

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003mars.conf.3194h&link_type=abstract

Sixth International Conference on Mars, July 20-25 2003, Pasadena, California, abstract no.3194

Physics

2

Scientific paper

Optical constants for martian dust have been extracted from Mariner 9
IRIS spectra to study sensitivity to particle opacity and size
distribution. Now, a large number of IRIS spectra over dusty areas is
being analyzed using full surface emissivity, in search of variations in
the dust properties.

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