@inproceedings{oai:jaxa.repo.nii.ac.jp:00020291,
 author = {宮本, 英昭 and Sato, Taketo and Miyamoto, Hideaki and Rodriguez, Alexis},
 book = {Proceedings of the 44th ISAS Lunar and Planetary Symposium},
 month = {},
 note = {44th  ISAS Lunar and Planetary Symposium (August 1-3,  2011. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan, Outflow channel is known as a water-related feature formed mainly on Hesperian terrains and is is expected to give a key to understand surface condition at that time. Large sized outflow channels like a Kasei Valles were argued well about their formation processes. Therefore we targeted Hebrus Valles and and Hephaestus Fossae as small sized outflow channels, and argued about their formation processes by estimating their discharge. We developed a simple method to calculate parameters necessary to estimate the discharge. As a result of discharge analysis we found that each formation process is different., 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: AA0065390006},
 publisher = {宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS), Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)},
 title = {Formation process of outflow channel located around Hebrus Valles},
 volume = {44},
 year = {2011}
}