@inproceedings{oai:jaxa.repo.nii.ac.jp:00020536,
 author = {荒井, 武彦 and 山本, 幸生 and 岡田, 達明 and 白井, 慶 and 小川, 和律 and 細野, 梢 and 加藤, 學 and Arai, Takehiko and Yamamoto, Yukio and Okada, Tatsuaki and Shirai, Kei and Ogawa, Kazunori and Hosono, Kozue and Kato, Manabu},
 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 = {The X-Ray fluorescence Spectrometers (XRS) onboard SELENE (SELenological and ENgineering Explorer) will globally and quantitatively determine the major elemental composition of lunar surface such as Mg, Al, Si, Ca, Ti, and Fe in the energy-range of 0.7 to 10.0 keV. This observation allows to construct lunar element and rock-type maps, and to study the lunar origin and evolution. In this study, we derived predicted spectra in order to construct deconvolution method with chi square fits, and simulated variations of these spectra in sync with solar activity. These systematic and analytic errors are at most 10 percent., 資料番号: AA0063350021},
 pages = {80--83},
 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 = {Simulation of lunar X-ray observation for XRS onboard SELENE},
 year = {2006}
}