講演情報
[PEM06-11]Structure of the magnetopause observed by MMS and its effects on the Kelvin-Helmholtz instability
*関 華奈子1、松本 洋介2、北村 成寿3、斎藤 義文3、横田 勝一郎3、星野 真弘1、Pollock Craig J.4,5、Giles Barbara L.5、Moore Thomas E.5、Torbert Roy B.6、Russell Christopher T.7、Burch James L.8 (1.東京大学大学院理学系研究科、2.千葉大学大学院理学研究科、3.JAXA宇宙科学研究所、4.Denali Scientific、5.NASA Goddard Space Flight Center、6.University of New Hampshire、7.University of California, Los Angeles、8.Southwest Research Institute)
キーワード：
magnetopause、boundary layer、Kelvin-Helmholtz Instability、plasma mixing、density gradient、MMS
How to cause plasma mixing across different plasma regimes has been one of the fundamental problems in the collisionless plasma physics. At a plasma boundary where different plasma regimes are in contact, there often exists a velocity shear and a density gradient. The Kelvin-Helmholtz instability (KHI) has been studied as a promising mechanism to cause the plasma mixing. Although the importance of the density gradient in the plasma transport acress the Earth’s magnetopause has previously been pointed out, the detailed structure of the boundary remains unknown due to lack of high-cadence observations across the magnetopause. Based on high time-resolution observations of ions and electrons as well as simultaneous magnetic field by MMS, we investigated the relations between the density gradient and velocity shear at the magnetopause. Based on the observed structure, we implemented a new initial condition for KHI simulations, and effects of the boundary structure on KHI excitation and subsequent plasma mixing is discussed.