@inproceedings{oai:jaxa.repo.nii.ac.jp:00020667,
 author = {石井, 徹之 and 佐々木, 晶 and Ishii, Tetsuyuki and Sasaki, Sho},
 book = {第36回月・惑星シンポジウム, Proceedings of the 36th ISAS Lunar and Planetary Symposium},
 month = {Nov},
 note = {The observation of recent gullies related to a possibility of the existence of liquid water on present Mars has been concerned in recent years. Some models assume formation of gullies by liquid water but they cannot explain the absence of the features in the equator regions. Other models assume CO2 as a volatile associated with the formation of gullies. It is shown that a latitude of the boundary between regions with CO2 consolidation on poleward-facing slops and those without CO2 condensation is about a latitude of 30 deg. The result suggests a possibility of some correlation between the existence of CO2 and the formation of gullies., 資料番号: AA0046650018},
 pages = {69--72},
 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 = {Temperature constraint on formation mechanism of recent gullies on Mars},
 year = {2003}
}