*Denis Pavel Cabezas1,3、Ayumi Asai2、Satoru UeNo3 (1.Department of Astronomy, Kyoto University、2.Unit of Synergetic Studies for Space, Kyoto University、3.Kwasan and Hida Observatories, Kyoto University)
セッション情報
[EE] ポスター発表
セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境
[P-EM18] [EE] Origin of Earth-affecting Coronal Mass Ejections
2017年5月24日(水) 15:30 〜 17:00 ポスター会場 (国際展示場 7ホール)
コンビーナ:No? Lugaz(University of New Hampshire Main Campus)、草野 完也(名古屋大学宇宙地球環境研究所)、Neel P Savani(NASA GSFC / University of Maryland Baltimore County)、浅井 歩(京都大学大学院理学研究科附属天文台)
Coronal mass ejections (CMEs) and CME-driven shocks and sheath regions are the primary drivers of strong geo-effective response, including geomagnetic storms, sudden impulse and changes in Earth's radiation belts. This session investigates the solar, coronal and interplanetary conditions under which fast and strong CMEs form and propagate, as well as the important characteristics to understand the solar wind-magnetosphere coupling and the variations in the radiation belts during the passage of a CME. Abstracts are solicited that focus on the type of active regions and solar conditions resulting in fast and strong CMEs, the interaction of CMEs with solar wind streams and other CMEs that affect their geo-effectiveness, the characteristics of CMEs and shocks that create strong sudden impulses and changes in the flux of energetic particles in Earth's radiation belts. Contributions that cover integrated investigations combining remote observations, numerical simulations and/or in situ measurements are especially welcome.
*Bin Zhuang1、Yuming Wang1、Chenglong Shen1、Siqing Liu2、Jingjing Wang2 (1.University of Science and Technology of China、2.National Space Science Center, CAS)
*Neel P Savani1、Angelos Vourlidas2 (1.NASA GSFC / UMBC、2.JHU APL)