日本地球惑星科学連合2019年大会

講演情報

[E] 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-EM11] Dynamics of Magnetosphere and Ionosphere

2019年5月29日(水) 17:15 〜 18:30 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、堀 智昭(名古屋大学宇宙地球環境研究所)

[PEM11-P05] Effects of the dipole tilt and the interplanetary magnetic field Bx component on the dawn-dusk and interhemispheric asymmetries of the interchange convection cycle

*渡辺 正和1,2田中 高史2藤田 茂3,4 (1.九州大学大学院理学研究院、2.九州大学国際宇宙天気科学・教育センター、3.気象大学校、4.国立極地研究所)

キーワード:電離圏対流、交換型磁力線再結合、リシプロカルセル

The interchange cycle is a mode of magnetic flux circulation that appears for periods of northward interplanetary magnetic field (IMF). It is made up of IMF-to-open reconnection in one hemisphere and open-to-closed reconnection in the other hemisphere. The two reconnection processes have the same topological nature in that the roles of the two reconnecting field lines interchange at the time of reconnection. The interchange cycle is characterized by reciprocation of open magnetic flux between the two hemispheres. One observable signature of the interchange cycle is an appearance of a reverse cell circulating in the closed field line region of the ionosphere, which is named the “reciprocal cell.” The reciprocal cell appears in the open-to-closed reconnection hemisphere, whereas in the opposite IMF-to-open reconnection hemisphere, there appears a lobe cell circulating exclusively on open field lines. For given (1) IMF By, (2) IMF Bx, and (3) dipole tilt conditions, two interchange cycles concur, one on the dawnside and the other on the duskside. For an ideal case, one can easily expect the mode of the interchange cycles to occur. For example, for the case of due northward IMF with significant dipole tilt, the twin reverse cells in the summer hemisphere are both lobe cells, while in the winter hemisphere the twin reverse cells are both reciprocal cells. For the general case, however, one cannot predict the mode of the interchange cycles without quantitative modeling. The purpose of this study is to examine how the presence of dipole tilt or IMF Bx alters the dawn-dusk and north-south pattern of the twin reverse cells. For this purpose, we perform numerical magnetohydrodynamic simulations using the REPPU (Reproduce Plasma Universe) code developed by T. Tanaka. In the presentation, we discuss the dipole tilt and IMF Bx effects revealed by the numerical modeling.