@inproceedings{oai:jaxa.repo.nii.ac.jp:00020452,
 author = {杉山, 耕一朗 and 小高, 正嗣 and 中島, 健介 and 林, 祥介 and Sugiyama, Koichiro and Odaka, Masatsugu and Nakajima, Kensuke 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 = {We develop a two-dimensional fluid dynamical model that incorporates condensation of H2O and NH3 and the production reaction of NH4SH. We run the model for a long simulation time in order to examine the structure of moist convection layer in Jupiter's atmosphere established through a large number of life cycles of convective clouds. Our results show that H2O and NH4SH cloud particles are advected to altitudes above the NH3 condensation level. The convective motion and the distribution of condensible species depend on the deep tropospheric mixing ratios of condensible volatiles., 資料番号: AA0063723032},
 pages = {137--140},
 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 = {Numerical modeling of moist convection in Jupiter's atmosphere: The dependency on the abundances of condensible volatiles},
 year = {2007}
}