@inproceedings{oai:jaxa.repo.nii.ac.jp:00020571,
 author = {土屋, 史紀 and 三澤, 浩昭 and Berezhnoy, A. and Tsuchiya, Fuminori and Misawa, Hiroaki and Berezhnoy, A.},
 book = {第38回月・惑星シンポジウム, Proceedings of the 38th ISAS Lunar and Planetary Symposium},
 month = {Mar},
 note = {Observations of lunar radio emission were carried out at the frequency of 325 MHz during the Perseids on August 11-13, 2004 in order to confirm the presence of lunar radio emission caused by meteoroid impacts with the moon and search for the emission mechanism of the lunar radio emission. On August 11, and 12, it was found that the antenna temperature of the moon increased by 3 K which was greater than the uncertainty of the temperature estimated to be about 1.5 K in the worst case. Further observations of the moon are planned to reveal detail characteristics of the lunar radio emission caused by meteoroid impacts., 資料番号: AA0063350056},
 pages = {208--211},
 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 = {Search for lunar radio emissions caused by meteoroid impacts: Radio observation at 325 MHz during the Perseids in Aug. 2004},
 year = {2006}
}