@inproceedings{oai:jaxa.repo.nii.ac.jp:00020488,
 author = {児玉, 信介 and 今村, 雄一郎 and 岩崎, 晃 and 中村, 良介 and 山口, 靖 and Kodama, Shinsuke and Imamura, Yuichiro and Iwasaki, Akira and Nakamura, Ryosuke and Yamaguchi, Yasushi},
 book = {第39回月・惑星シンポジウム, Proceedings of the 39th ISAS Lunar and Planetary Symposium},
 month = {Aug},
 note = {The ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer) VNIR (Visible and Near Infrared) and SWIR (Short Wave Infrared) lunar imageries were used to derive the bidirectional reflectance of the lunar surface and used for mineralogical mapping. The average reflectance at the Apollo 16 landing site was 8.6 percent in the visible, and 18.6 percent in the near infrared region at standard geometry (i = 30, e = 0, alpha = 30), which are lower (0.5-0.55 times) than those of the Apollo sample (62231). Our result is consistent with the results from the observation using Earth based telescope (0.53 in the visible region), suggesting that the reflectance of the Apollo sample derived in the laboratory is higher than that of the lunar surface., 資料番号: AA0063505026},
 pages = {100--103},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Lunar surface observation with ASTER onboard Terra},
 year = {2006}
}