A visible and near-infrared photometric correction for Moon Mineralogy Mapper (M3)

Author:

Besse S.,Sunshine J.,Staid M.,Boardman J.,Pieters C.,Guasqui P.,Malaret E.,McLaughlin S.,Yokota Y.,Li J.-Y.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference34 articles.

1. Besse, S. et al., 2011a. Lunar optical remote sensing measurements: Quantitative comparisons of M3 and SIR-2 on Chandrayaan-1 and SP and MI on Kaguya. Presented at the EPSC-DPS Joint Meeting 2011, held 2–7 October 2011 in Nantes, France, p. 1865. .

2. Besse, S. et al., 2011b. Deriving a photometric model for the Moon Mineralogy Mapper data (M3). Lunar Planet. Sci., 1773 (abstracts).

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. (Planets),2011

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

5. Lunar Reconnaissance Orbiter overview: The instrument suite and mission;Chin;Space Sci. Rev.,2007

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