Optical Response and Surface Physical Properties of the Lunar Regolith at Reiner Gamma Formation from Clementine Orbital Photometry: Derivation of the Hapke Parameters at Local Scale

Details Optical Response and Surface Physical Properties of the Lunar Regolith at Reiner Gamma Formation from Clementine Orbital Photometry: Derivation of the Hapke Parameters at Local Scale Optical Response and Surface Physical Properties of the Lunar Regolith at Reiner Gamma Formation from Clementine Orbital Photometry: Derivation of the Hapke Parameters at Local Scale

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1660p&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1660

Physics

11

Scientific paper

The set of Hapke parameters is derived for the Reiner Gamma area at 900m
resolution using Clementine multiangular imaging; the local photometric
variations seen are consistent with the plowing of the regolith by a
swarm of cometary fragments.

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