@inproceedings{oai:jaxa.repo.nii.ac.jp:00038420,
 author = {岡田, 達明 and 田中, 智 and 飯島, 祐一 and 藤村, 彰夫 and 水谷, 仁 and 加藤, 學 and 鳥居, 龍晴 and 鈴木, 和司 and 増田, 忠志 and Okada, Tatsuaki and Tanaka, Satoshi and Iijima, Yuichi and Fujimura, Akio and Mizutani, Hitoshi and Kato, Manabu and Torii, Tatsuharu and Suzuki, Kazuji and Masuda, Tadashi},
 book = {第28回月・惑星シンポジウム, Proceedings of the 28th ISAS Lunar and Planetary Symposium},
 month = {Dec},
 note = {X-ray fluorescence spectrometer using a large-area Gas Scintillation Proportional Counter (GSPC) is being developed for the future planetary explorations such as the asteroid-sample-return mission and the lunar remote-sensing missions both proposed in Japan. As was proven in the Apollo missions, surface major elemental composition can be quantitatively determined through XRF (X-Ray Fluorescence) spectrometry from orbiters. We manufactured two GSPC testing models and carried out laboratory experiments to examine its performance. On the basis of the experimental results, we propose here a basic design of improved XRF spectrometer, which could be applicable to asteroid, lunar, and other planetary missions., 資料番号: AA0063352053},
 pages = {197--200},
 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 = {Development of X-ray fluorescence spectrometer using a large-area GSPC},
 year = {1995}
}