日本地球惑星科学連合2022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-EM10] Dynamics of Magnetosphere and Ionosphere

2022年6月2日(木) 11:00 〜 13:00 オンラインポスターZoom会場 (5) (Ch.05)

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:佐藤 由佳(日本工業大学)、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)、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)


11:00 〜 13:00

[PEM10-P06] Ion outflow from lobe reconnection and its relation to shear flow

*小池 春人1田口 聡1 (1.京都大学大学院理学研究科地球惑星科学専攻地球物理学教室太陽惑星系電磁気学講座)

キーワード:マグネトポーズ、ローブリコネクション、シアフロー

One of the important topics for magnetic reconnection is the role of shear flow which flows parallel to the reconnecting field. Previous simulation studies have suggested that shear flow reduces the reconnection rate and the outflow speed. Further studies need be done from observations to understand the role of shear flow in reconnection deeply. For reconnection at the high-latitude magnetopause during northward IMF, the magnetosheath flow streaming tailward acts as shear flow. In this study, we took the lobe reconnection events observed by the Cluster satellites, and examined relationships of the ion outflow to the magnetosheath tailward flow. The result from the statistical analysis has shown that there is a tendency for the ion outflow to increase as the speed of the magnetosheath flow increases. This indicates that ions are more greatly accelerated through the lobe reconnection as shear flow streams faster. This tendency seems to be inconsistent with the result from the previous simulation studies. We will discuss this discrepancy in terms of additional acceleration by the Hall electric field in the ion diffusion region.