Examination of the Most Diagnostic Spectral Regions From Visible Through Thermal Infrared for Polar Studies of Mars

Details Examination of the Most Diagnostic Spectral Regions From Visible Through Thermal Infrared for Polar Studies of Mars Examination of the Most Diagnostic Spectral Regions From Visible Through Thermal Infrared for Polar Studies of Mars

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998lpico.953...16h&link_type=abstract

The First International Conference on Mars Polar Science and Exploration, Proceedings of the Conference held at Camp Allen, TX.

Computer Science

Dust, Ice, Mars (Planet), Mars Surface, Polar Caps, Carbon Dioxide, Clouds, Ice Clouds, Infrared Radiation, Thermal Radiation, Infrared Radiometers, Infrared Spectrometers

Scientific paper

Many outstanding polar questions can be examined using data returned by spacecraft instruments that record either multiband measurements or spectra from visible or infrared wave-lengths. Here we discuss which spectral regions provide the most diagnostic information to address the following polar questions: (1) seasonal and perennial ice cap composition; (2) ice grain sizes and/or layer thicknesses; (3) fractional coverage of the ground by ice, and mixtures of ices with dust or soil, (4) radiative balance; (5) non-ice surface composition; and (6) presence and composition of clouds. To make the discussion more manageable, we divide the spectral ranges into four convenient groups: visible only; near-infrared (about 0.8-5 microns); thermal infrared (-5-50 microns); and near-through-thermal infrared (-0.8-50 microns).

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