@inproceedings{oai:jaxa.repo.nii.ac.jp:00020687,
 author = {児玉, 信介 and 山口, 靖 and Kodama, Shinsuke and Yamaguchi, Yasushi},
 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 = {For the purpose of understanding the temporal and spatial variations of lunar mare volcanism, the mare basalts on the lunar nearside were mapped, and their stratigraphy was established for each mare region using the Clementine UVVIS data. The mare basalts are younger in the western maria than in the eastern maria in a global scale, whereas northern mare units tend to be younger than southern mare units in a local scale. The high-Ti basalts tend to erupt in the latter stages in each region, and this fact suggests that a similar magma generation process might exist in the source regions of these maria., 資料番号: AA0046650038},
 pages = {149--152},
 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 = {Mare volcanism in the nearside of the moon inferred from Clementine UVVIS data},
 year = {2003}
}