日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(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-EM06] Magnetospheric Multi-Scale (MMS) mission -- A new age of magnetospheric physics

2016年5月24日(火) 09:00 〜 10:30 103 (1F)

コンビーナ:*銭谷 誠司(国立天文台)、北村 成寿(宇宙航空研究開発機構 宇宙科学研究所)、斎藤 義文(宇宙航空研究開発機構・宇宙科学研究所・太陽系科学研究系)、Paul Cassak(West Virginia University)、Chen Li-Jen(NASA Goddard Space Flight Center)、Craig Pollock(NASA Goddard Space Flight Center)、座長:Oka Mitsuo(University of California Berkeley)、銭谷 誠司(国立天文台)

10:00 〜 10:15

[PEM06-05] Magnetic energy dissipation of plasma sheet under coupling of magnetic reconnection and lower hybrid drift instability

★招待講演

*星野 真弘1 (1.東京大学大学院理学系研究科)

キーワード:magnetic reconnection, plasma sheet, palsma heating, lower hybrid drift instability

Understanding of the magnetic energy dissipation process in a current sheet is an important problem in space plasma as well as in MMS science. So far the inertia resistivity by reconnection and the current driven instability such as the lower hybrid drift instability (LHDI) have been discussed as possible candidates for the origin of microscopic process of magnetic energy dissipation. It is well known that while the LHDI is mainly excited in the plasma sheet boundary, the inertia resistivity effectively works at the neutral sheet. Therefore, the role of the LHDI to the magnetic field dissipation is less important than the inertia resistivity involved in the magnetic reconnection. However, the activity of lower hybrid drift waves together with the electron heating is commonly observed in the plasma sheet boundary by modern satellite observations, and their impact on the magnetic field dissipation at the neutral sheet is not necessarily neglected. In addition, the nonlinear coupling between them is not theoretically understood yet. In this talk, we study the coupling of the collisionless reconnection and the LHDI by using a three-dimensional PIC simulation by paying a special attention to electron heating and the magnetic energy dissipation, and discuss the importance of the current driven instability during magnetic reconnection.