planetary magnetosphere, solar prominence, solar flare, solar corona, magnetic disturbance, solar cycle, solar activity, latitudinal variation, interplanetary space, photosphere
Miyagi University of Education
Miyagi University of Education
Miyagi University of Education
Solar-Terrestrial Environment Laboratory, Nagoya University
Solar-Terrestrial Environment Laboratory, Nagoya University
出版者
宇宙航空研究開発機構宇宙科学研究本部
出版者（英）
Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)
雑誌名
第28回月・惑星シンポジウム
雑誌名(英)
Proceedings of the 28th ISAS Lunar and Planetary Symposium
ページ
141 - 144
発行年
1995-12
抄録（英）
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.
Disturbance sources of planetary magnetospheres and latitudinal variation of solar prominence
