| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1773854 | Icarus | 2011 | 22 Pages |
Abstract
⺠We derived lunar photometric correction parameters for wavelengths 0.5-1.6 μm. ⺠We obtained different parameter sets for three albedo groups. ⺠The parameters cover solar phase angles between 5° and 85°. ⺠An additional correction method for high latitude regions was investigated. ⺠The lunar high latitude regions have bluer spectra than the other regions.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Yasuhiro Yokota, Tsuneo Matsunaga, Makiko Ohtake, Junichi Haruyama, Ryosuke Nakamura, Satoru Yamamoto, Yoshiko Ogawa, Tomokatsu Morota, Chikatochi Honda, Kazuto Saiki, Kenichi Nagasawa, Kohei Kitazato, Sho Sasaki, Akira Iwasaki, Hirohide Demura,