@inproceedings{oai:jaxa.repo.nii.ac.jp:00020453,
 author = {石渡, 正樹 and 中島, 健介 and 森川, 靖大 and 高橋, 芳幸 and 小高, 正嗣 and 倉本, 圭 and 林, 祥介 and Ishiwatari, Masaki and Nakajima, Kensuke and Morikawa, Yasuhiro and Takahashi, Yoshiyuki O. and Odaka, Masatsugu and Kuramoto, Kiyoshi and Hayashi, Yoshiyuki},
 book = {第40回月・惑星シンポジウム, Proceedings of the 40th ISAS Lunar and Planetary Symposium},
 month = {Jul},
 note = {A numerical experiment on the climate state of a synchronously rotating terrestrial planet is performed by using a General Circulation Model (GCM) with simplified hydrologic and radiative processes. The system utilized is basically equivalent to the GCM of Ishiwatari et al. (2002) in which the runaway greenhouse state in a three-dimensional system is examined. The value of solar constant is set to the terrestrial value. The incident solar radiation is assumed to be permanently given to one side of planet. The results of the experiment are as follows: (1) Longitudinal heat transport in low latitudinal region is resulted from propagations of equatorial Kelvin wave and equatorial Rossby wave. (2) In higher latitudinal region, baroclinic eddies contribute to heat transport from the day side to the night side., 資料番号: AA0063723033},
 pages = {141--146},
 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 = {A numerical experiment on atmospheric circulation of a synchronously rotating planet},
 year = {2007}
}