@inproceedings{oai:jaxa.repo.nii.ac.jp:00020596,
 author = {岡田, 靖彦 and 浅田, 章大 and 野村, 英子 and 浦川, 聖太郎 and 中村, 吉宏 and 向井, 正 and Okada, Yasuhiko and Asada, Akihiro and Nomura, Hideko and Urakawa, Seitaro and Nakamura, Yoshihiro and Mukai, Tadashi},
 book = {第37回月・惑星シンポジウム, Proceedings of the 37th ISAS Lunar and Planetary Symposium},
 month = {Feb},
 note = {Temperature of irregularly shaped dust particles radiated by the sun is considered. As the calculation method of absorption cross section of the dust, MG-Mie method is used. MG-Mie method shows good agreement for the result with DDA (Discrete Dipole Approximation) in the range where the DDA method can be used to calculate the optical properties accurately only with a few percentage error. The difference in the particle shape causes difference of the dust temperature in terms of size dependence and of spatial distribution as the results of different optical properties., 資料番号: AA0047898018},
 pages = {69--72},
 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 = {Temperature distribution of dust particles with irregular shapes},
 year = {2004}
}