@inproceedings{oai:jaxa.repo.nii.ac.jp:00020581,
 author = {鈴木, 絢子 and 熊谷, 一郎 and 永田, 裕作 and 栗田, 敬 and Suzuki, Ayako and Kumagai, Ichiro and Nagata, Yusaku and Kurita, Kei},
 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 = {Martian pedestal craters have many interesting morphologies on their ejecta blankets. It has been considered that fluidized ejecta generate these features. Here laboratory analogue experiments have been conducted to examine the atmospheric effects on the ejecta emplacement of pedestal craters. The experimental results show that modified morphologies are divided into three modes by critical parameter. Physical constraints are discussed for the atmospheric conditions in which grooves on the surface of Martian pedestal crater are carved., 資料番号: AA0047898003},
 pages = {9--12},
 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 = {Laboratory experiments on Martian pedestal craters: Interaction between a vortex ring and a layer of small particles},
 year = {2004}
}