@inproceedings{oai:jaxa.repo.nii.ac.jp:00020359,
 author = {佐々木, 晶 and 石原, 吉明 and 荒木, 博志 and 野田, 寛大 and 花田, 英夫 and 松本, 晃治 and 並木, 則行 and 岩田, 隆浩 and 杉田, 精司 and Sasaki, Sho and Ishihara, Yoshiaki and Araki, Hiroshi and Noda, Hirotomo and Hanada, Hideo and Matsumoto, Koji and Goossens, Sander and Namiki, Noriyuki and Iwata, Takahiro and Sugita, Seiji},
 book = {月・惑星シンポジウム, Proceedings of the ISAS lunar and planetary symposium},
 month = {Aug},
 note = {第42回 月・惑星シンポジウム(2009年8月5-7日, 宇宙航空研究開発機構宇宙科学研究本部), The 42nd ISAS Lunar and Planetary Symposium (August 5-7, 2009. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan, Gravity and topography data obtained by KAGUYA (SELENE) are used to characterize the structure of South Pole-Aitken basin of the Moon. Previously proposed elliptic basin shape was confirmed by the revised topography and Moho depth (and crustal thickness) distribution by KAGUYA. Moho depth just outside the SPA basin is about 50-70 km, whereas Moho at the central region of SPA is as shallow as 30 km., 形態: カラー図版あり, 形態: CD-ROM1枚, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0064739015},
 pages = {63--66},
 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)},
 title = {Shape and Structure of the Lunar South Pole-Aitken Basin from KAGUYA(SELENE) Gravity/Topography},
 volume = {42},
 year = {2009}
}