Hapke modeling of Rhea surface properties through Cassini-VIMS spectra

Details Hapke modeling of Rhea surface properties through Cassini-VIMS spectra Hapke modeling of Rhea surface properties through Cassini-VIMS spectra

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..214..541c&link_type=abstract

Icarus, Volume 214, Issue 2, p. 541-555.

Physics

2

Scientific paper

Rhea's spectrum and phase function modeling. Spectra
from VIMS on board Cassini spacecraft. Intraparticle mixture of
water ice and Triton tholin reproduces observed reddening. Determination of phase function parameters. Dependence of phase
function parameters on single scattering albedo.

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