@inproceedings{oai:jaxa.repo.nii.ac.jp:00038405,
 author = {齋藤, 尚生 and 森, 洋介 and 安江, 正治 and 松浦, 善博 and 小塚, 幸央 and 小島, 正宜 and Saito, Takao and Mori, Yosuke and Yasue, Masaharu and Matsuura, Yoshihirio and Kozuka, Yukio and Kojima, Masayoshi},
 book = {第28回月・惑星シンポジウム, Proceedings of the 28th ISAS Lunar and Planetary Symposium},
 month = {Dec},
 note = {Three solar sources (flare, coronal hole, and filament disappearance) of planetary magnetosphere disturbances are studied in relation to the large-scale magnetic structure of the sun. Peculiar latitudinal variation observed in dark filaments, namely prominences, are well explained by a relation with the tree-dimensional magnetic structure. In conclusion all the three solar sources are revealed to have systematic relations with the source-surface neutral line., 資料番号: AA0063352038},
 pages = {141--144},
 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 = {Disturbance sources of planetary magnetospheres and latitudinal variation of solar prominence},
 year = {1995}
}