@inproceedings{oai:jaxa.repo.nii.ac.jp:00020297,
 author = {熊本, 篤志 and 小野, 高幸 and 寺田, 直樹 and 加藤, 雄人 and 山口, 靖 and 押上, 祥子 and Ishiyama, Ken and Kumamoto, Atsushi and Ono, Takayuki and Terada, Naoki and Kato, Yuto and Yamaguchi, Yasushi and Oshigami, Shoko},
 book = {Proceedings of the 44th ISAS Lunar and Planetary Symposium},
 month = {},
 note = {44th  ISAS Lunar and Planetary Symposium (August 1-3,  2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, The Lunar Radar Sounder (LRS) surveyed the lunar subsurface structure globally. The thickness of a stratum is significant in order to discuss the evolution of the lava flow flux in the lunar thermal history based on radar observations. The relative permittivity of the stratum is an important parameter to obtain the actual thickness of each lava flow unit. In this study, the relative permittivity of the upper basalt layer is investigated in Mare Imbrium, Mare Crisium, and Oceanus Procellarum by applying the new analysis method based on the comparison between radar sounder data and terrain camera data. The relative permittivity in analysis areas is obtained as 2.7+/-0.5. On the basis of new analysis method, we study the permittivity of the upper basalt layer having the thickness of a few hundred meters., 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: AA0065390012},
 publisher = {宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS), Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)},
 title = {An estimation method of the lunar surface permittivity based on the observation equipments onboard Kaguya spacecraft (SELENE)},
 volume = {44},
 year = {2011}
}