日本地球惑星科学連合2022年大会

講演情報

[E] 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-EM10] Dynamics of Magnetosphere and Ionosphere

2022年5月26日(木) 09:00 〜 10:30 303 (幕張メッセ国際会議場)

コンビーナ:佐藤 由佳(日本工業大学)、コンビーナ:家田 章正(名古屋大学 宇宙地球環境研究所)、藤本 晶子(九州工業大学)、コンビーナ:今城 峻(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)、座長:長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、西野 真木(宇宙航空研究開発機構宇宙科学研究所)


10:15 〜 10:30

[PEM10-05] Evolution of electrostatic potential in magnetosphere-ionosphere system as simulated by global MHD model with Alfvénic-coupling

*中溝 葵1吉川 顕正2中田 裕之3深沢 圭一郎4田中 高史2 (1.情報通信研究機構電磁波研究所、2.九州大学大学院理学研究院、3.千葉大学大学院工学研究院、4.京都大学学術情報メディアセンター)

キーワード:磁気圏電離圏結合、Alfvenic結合アルゴリズム、グローバル磁気圏MHDシミュレーション、電離圏電気伝導度

By using the Polarization Field Separation method [Nakamizo and Yoshikawa, 2019] and a global MHD model [Tanaka, 2015], we have shown that the ionosphere plays an active role in the configuration and dynamics of the global magnetosphere due to its non-uniform conductance distribution. The feedback process from the ionosphere to the magnetosphere in the current global MHD simulations can be described as follows; (1) The ionospheric conductance non-uniformity generates polarization fields, thereby deforming the ionospheric electric potential pattern. (2) The information of deformation is reflected in the magnetospheric bulk velocity updated by the potential mapped back to the magnetospheric inner boundary (Vperp=-(ExB)/B2). (3) The updated velocity disturbances propagate the magnetosphere, modifying the force and energy balance of MHD field. (4) The FAC distribution at the next time step is calculated in the magnetosphere updated in this way and is inputted again to the ionosphere, generating the ionospheric potential of the next time step. (5) Thus, the effect of ionospheric polarization fields is accumulatively included in the development of the magnetosphere–ionosphere system.

In order to investigate precisely the role of ionosphere, we implement Alfvénic-coupling algorithm proposed by Yoshikawa et al. [2010] in the MHD code. In the Alfvénic-coupling algorithm, both FACs and potential are mapped between the magnetosphere and ionosphere in terms of the incident and reflection process of shear Alfvén waves, therefore the continuities of physical quantities and the conservations of momentum and energy are ensured. As an implementation test, we show how the reflected FACs, reflected potential, and total (M-I coupled) potential change depending on the ratio of Pedersen conductance and Alfvén conductance. We also compare the total FACs, total potential, and velocity perturbations around the inner boundary obtained by the normal coupling and Alfvénic-coupling.