@inproceedings{oai:jaxa.repo.nii.ac.jp:00038423,
 author = {寺薗, 淳也 and 滝沢, 悦貞 and 金子, 豊 and 大嶽, 久志 and 汲田, 啓一 and 俣野, 米治 and 神原, 洋 and 三箇, 智二 and Terazono, Junya and Takizawa, Yoshisada and Kaneko, Yutaka and Otake, Hisashi and Kumita, Keiichi and Matano, Yoneharu and Kanbara, Hiroshi and Sanga, Tomoji},
 book = {第28回月・惑星シンポジウム, Proceedings of the 28th ISAS Lunar and Planetary Symposium},
 month = {Dec},
 note = {We analyzed multi-spectral lunar surface images which were taken by Clementine satellite to evaluate the possibility for recognition of lunar surface geology. Images obtained by the Ultraviolet-Visible camera (UVVIS) are analyzed. Our analysis could distinguish nine geological regions, six for the mare and three for the highland., 資料番号: AA0063352056},
 pages = {209--212},
 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 geology analysis using image data obtained by Clementine},
 year = {1995}
}