Regolith Radiative Transfer Model

Details Regolith Radiative Transfer Model Regolith Radiative Transfer Model

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006dps....38.4211v&link_type=abstract

American Astronomical Society, DPS meeting #38, #42.11; Bulletin of the American Astronomical Society, Vol. 38, p.561

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We are developing an improved regolith radiative transfer model (RRT) for multiple applications in planetary systems. Our immediate motivation for developing this particular RRT model is new data from Cassini at long IR wavelengths (100-500 microns). The first application will be to simulate the emissivity of the ring's grainy regoliths at far infrared wavelengths. The behavior of the emissivity at far IR is an important probe for determining the composition of the non-icy components of ring material.

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