日本地球惑星科学連合2018年大会

講演情報

[EE] 口頭発表

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-EM13] 太陽地球系結合過程の研究基盤形成

2018年5月20日(日) 13:45 〜 15:15 304 (幕張メッセ国際会議場 3F)

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所、共同)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:吉川 顕正山本 衛

14:30 〜 14:45

[PEM13-14] Research project for investigation of active role of ionospheric dynamics on the magnetosphere-ionosphere coupled system

*吉川 顕正1,2大谷 晋一3中溝 葵4今城 峻5 (1.九州大学大学院理学研究院地球惑星科学部門、2.九州大学国際宇宙天気科学・教育センター、3.ジョンズ・ホプキンス大学応用物理学研究所、4.情報通信研究機構、5.京都大学大学院理学研究科附属地磁気世界資料解析センター)

キーワード:磁気圏電離圏結合、電離圏の能動的役割

Ionospheric Hall effect strongly controls spatiotemporal evolution of Magnetosphere-Ionosphere (MI) coupling system.

Generation of polarization electric field at the conductivity gradient region causes rotation, shear, and acceleration and deceleration of ionospheric convection field in both local and global manners. The ionospheric polarization field activates upward shear Alfven wave that could cause ionospheric driven magnetospheric dynamics and induce new type of MI coupled current system.

Generation of induction electric field at the wave front of ionospheric disturbances enable to horizontally propagate an electrostatic type electric field as a result of coupling between magnetosonic mode and shear Alfven mode at the ionospheric E-layer induced by multistep Hall effect in a time domain. Understanding a combined effect of ionospheric polarization and induction on the ionospheric dynamics becomes key element formation of global current system from polar to equatorial ionosphere.

To understand active role of ionospheric dynamics on the global MI-coupled system, we coordinate integrated study of theory, numerical simulation, global observation of ionospheric dynamics and satellite observation of magnetospheric aspects. In this talk, we will discuss what is essential physics of this project, how to identify elementary components from coupled phenomena, and how to coordinate integrated study for understanding active role of ionospheric dynamics.