A wavelength-dependent visible and infrared spectrophotometric function for the Moon based on ROLO data

被引：34

作者：

Buratti, B. J. ^{[1
]}

Hicks, M. D. ^{[1
]}

Nettles, J. ^{[2
]}

Staid, M. ^{[3
]}

Pieters, C. M. ^{[2
]}

Sunshine, J. ^{[4
]}

Boardman, J. ^{[5
]}

Stone, T. C. ^{[6
]}

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA

[3] Planetary Sci Inst, Tucson, AZ 85719 USA

[4] Univ Maryland, Dept Astron, College Pk, MD 20742 USA

[5] Analyt Imaging & Geophys, Boulder, CO 80303 USA

[6] USGS, Flagstaff, AZ 86001 USA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS | 2011年 / 116卷

基金：

美国国家航空航天局;

关键词：

BIDIRECTIONAL REFLECTANCE SPECTROSCOPY; SATELLITES; PHOTOMETRY; CLEMENTINE;

D O I：

10.1029/2010JE003724

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

The USGS's Robotic Lunar Observatory (ROLO) dedicated ground-based lunar calibration project obtained photometric observations of the Moon over the spectral range attainable from Earth (0.347-2.39 mu m) and over solar phase angles of 1.55 degrees-97 degrees. From these observations, we derived empirical lunar surface solar phase functions for both the highlands and maria that can be used for a wide range of applications. The functions can be used to correct for the effects of viewing geometry to produce lunar mosaics, spectra, and quick-look products for future lunar missions and ground-based observations. Our methodology can be used for a wide range of objects for which multiply scattered radiation is not significant, including all but the very brightest asteroids and moons.

引用

页数：8

共 25 条

[1] The lunar opposition surge: Observations by Clementine [J].