@inproceedings{oai:jaxa.repo.nii.ac.jp:00019940,
 author = {越後, 亮三 and 上宇都, 幸一 and Echigo, Ryosan and Kamiuto, Koichi},
 book = {太陽系科学シンポジウム: 講演集録},
 month = {},
 note = {第30回太陽系科学シンポジウム(2008年12月18日-19日, 宇宙航空研究開発機構宇宙科学研究本部), The thermal structure of lunar craters has been examined to reveal surface temperature and heat flux in the underground by taking account of radiation heat transfer between internal surfaces of crater wall. The boundary condition is formulated to be integro-differential equation for the radiant exchanges. Analytical results have illustrated that the temperature of crater wall is generally the same or rather lower compared with surrounding plain surface in comparatively lower altitude area and also disclosed that the prominent high temperature is yielded in the polar region due the cosine of incident radiation and the dominant annual cycle of heating., 形態: カラー図版あり, 資料番号: AA0064290020},
 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 = {月面におけるクレーターの熱構造解析},
 volume = {30},
 year = {2009}
}