日本地球惑星科学連合2024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

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

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)、家田 章正(名古屋大学 宇宙地球環境研究所)、佐藤 由佳(日本工業大学)、藤本 晶子(九州工業大学)

17:15 〜 18:45

[PEM10-P18] Advanced methods for analyzing in-situ observations of magnetic reconnection

*長谷川 洋1、ISSI team (1.JAXA宇宙科学研究所)

キーワード:磁気リコネクション、データ解析手法、拡散領域

Magnetic reconnection in planetary magnetospheres plays a pivotal role in the transfer of solar wind mass, momentum, and energy to the magnetosphere and rapid release of magnetic energy from the magnetotail during magnetospheric substorms or explosive auroral activity. It is, however, a nontrivial task to identify, visualize, and elucidate the physical processes at work in reconnection regions from in-situ measurements of plasma particles and electromagnetic fields. Here, an overview is given of how reconnection effects or regions at global, magnetohydrodynamic-, ion-, and electron-scales can be identified and analyzed by use of in-situ measurements by space probes in and around Earth’s magnetosphere. A particular emphasis is placed on recent advances in the era of NASA's Magnetospheric Multiscale mission, which has made, since the launch in 2015, electron-scale, multi-point measurements in the near-Earth space of magnetic reconnection in the collisionless regime. The methodology for the identification and analysis includes a variety of single- and multi-spacecraft data analysis techniques that are key to revealing the context of in-situ observations of magnetic reconnection in space and for detecting and analyzing the diffusion regions where ions and/or electrons are demagnetized and magnetic energy is converted to plasma energy.