@inproceedings{oai:jaxa.repo.nii.ac.jp:00020399,
 author = {本田, 親寿 and 諸田, 智克 and 横田, 康弘 and 小川, 佳子 and 出村, 裕英 and 平田, 成 and 松永, 恒雄 and 大竹, 真紀子 and 春山, 純一 and Honda, Chikatoshi and Morota, Tomokatsu and Yokota, Yasuhiro and Ogawa, Yoshiko and Demura, Hirohide and Hirata, Naru and Matsunaga, Tsuneo and Ohtake, Makiko and Haruyama, Junichi},
 book = {Proceedings of the ISAS lunar and planetary symposium},
 month = {},
 note = {The 41st ISAS Lunar and Planetary Symposium (August 6-8, 2008. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)), We measured the morphologic characteristics such as depth and width of the Vallis Schroteri, and slope of the ground at which the rille exists. The change of depth profile as a function of distance from the vent-like feature supports that the cause of this rille is the thermal erosion of the flowing lava which has a low viscosity as same as komatiite lava flow on the Earth., Physical characteristics: Original contains color illustrations, 資料番号: AA0064291020},
 pages = {81--83},
 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 = {Morphologic characteristics of Vallis Schroteri on the Aristarchus plateau},
 volume = {41},
 year = {2009}
}