Lunar opposition effect as inferred from Chandrayaan-1 M3data

Author:

Kaydash Vadym1,Pieters Carle2,Shkuratov Yuriy1,Korokhin Viktor1

Affiliation:

1. Astronomical Institute of Kharkov V.N. Karazin National University; Kharkov Ukraine

2. Department of Geological Sciences; Brown University; Providence Rhode Island USA

Funder

NASA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference36 articles.

1. Akimov , L. A. I. I. Antipova-Karataeva Y. G. Shkuratov 1979 Indicatrix measurements of lunar samples from landing sites of Luna 24, Luna 16, and Luna 20

2. A visible and near-infrared photometric correction for Moon Mineralogy Mapper (M3);Besse;Icarus,2013

3. Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation, and related Level 1B products of the Moon Mineralogy Mapper;Boardman;J. Geophys. Res.,2011

4. The lunar opposition surge: observation by Clementine;Buratti;Icarus,1996

5. A wavelength-dependent visible and infrared spectrophotometric function for the Moon based on ROLO data;Buratti;J. Geophys. Res.,2011

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