@inproceedings{oai:jaxa.repo.nii.ac.jp:00020405,
 author = {川村, 太一 and 田中, 智 and 斎藤, 靖之 and 小林, 佑輔 and Kawamura, Taichi and Tanaka, Satoshi and Saito, Yasuyuki and Kobayashi, Yusuke and Hagermann, Axel},
 book = {Proceedings of the ISAS lunar and planetary symposium},
 month = {},
 note = {The 41st ISAS Lunar and Planetary Symposium (August 6-8, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), The internal structure of the Moon is an essential piece of information that infer the origin and evolution of the Moon. Many attempts have been made for its estimation and seismic analysis using the data from Apollo Passive Seismic Experiment (PSE) is one of the most successful methods carried out. We have been focusing on the possibility of seismic use of the Lunar Surface Gravimeter (LSG) data of Apollo 17. In this study we dealt with seismic analysis of deep moonquakes and searched for possibility of the seismic use of the LSG data for deep moonquakes. We examined events from source regions A01, A06, A07, and A22. We found that 38 events out of 99 events were detected by the LSG. With 31 events, we also constructed travel time curves and tested the estimation and classification of previous study. Our result supported the previous result. We also examined some unclassified events and found events that were detected by the LSG. The detection of the signals implies the possibility of classification of unclassified events using the LSG., 資料番号: AA0064291026},
 pages = {105--113},
 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 = {Re-analysis of deep moonquakes using the Lunar Surface Gravimeter},
 volume = {41},
 year = {2009}
}