@inproceedings{oai:jaxa.repo.nii.ac.jp:00020367,
 author = {越後, 亮三 and Echigo, Ryosan},
 book = {月・惑星シンポジウム, Proceedings of the ISAS lunar and planetary symposium},
 month = {Aug},
 note = {第42回 月・惑星シンポジウム(2009年8月5-7日, 宇宙航空研究開発機構宇宙科学研究本部), The 42nd ISAS Lunar and Planetary Symposium (August 5-7, 2009. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), Sagamihara, Kanagawa Japan, The harbor water ice, deposited by comets or asteroids and preserved in the craters is premised on the very low temperature produced in the permanently shadowed portions of certain craters. One area of particular interest is Shackleton crater, located in the South Pole. An analysis is executed to calculate the temperature profiles throughout the basin by taking account of thermal radiation exchange based on a sophisticated physical model for the boundary condition consist of integro-differential equation. The numerical results exhibit an annual temperature change along the somma and the subsequently the related heat transfer mechanism is discussed through an entire region of crater., 形態: カラー図版あり, 形態: CD-ROM1枚, Physical characteristics: Original contains color illustrations, Note: One CD-ROM, 資料番号: AA0064739023},
 pages = {96--99},
 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 = {An Analysis on Radiation Heat Transfer into Permanent Shadow of Lunar Crater},
 volume = {42},
 year = {2009}
}