Department of Geophysics, University of Tohoku
Department of Geophysics, University of Tohoku
Department of Geophysics, University of Tohoku
Korea Institute of Geology, Mining and Materials (KIGAM)
Division of Earth and Planetary Sciences, Graduate School of Science, Kyoto University
Department of Earth and Planetary Sciences, Nagoya University
Department of Earth and Planetary Sciences, Nagoya University
LRS team member
出版者
宇宙航空研究開発機構宇宙科学研究本部
出版者（英）
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)
雑誌名
Proceedings of the ISAS lunar and planetary symposium
巻
41
ページ
59 - 62
発行年
2009
会議概要（会議名, 開催地, 会期, 主催者等）（英）
The 41st ISAS Lunar and Planetary Symposium (August 6-8, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA))
抄録（英）
To obtain information on the subsurface geological features of the Moon, the Lunar Radar Sounder (LRS) experiment has been carried out on-board the Kaguya spacecraft. LRS has successfully derived a global survey of the geological features of the lunar surface and subsurface region by applying the HF radar method. Here the global distributions of some characteristics such as the surface echo power, the duration time, the RMS gradient, and the integrated intensity have been investigated. These maps indicated a clear regional dependence in the mare region, the highland region, and the vicinity of the typical crater.
内容記述（英）
Physical characteristics: Original contains color illustrations
Global distribution of HF radar sounder echo derived from Kaguya/LRS
