JpGU-AGU Joint Meeting 2017

講演情報

[EE] 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-EM14] [EE] Dynamics in magnetosphere and ionosphere

2017年5月20日(土) 15:30 〜 17:00 105 (国際会議場 1F)

コンビーナ:堀 智昭(東京大学大学院理学系研究科)、田中 良昌(国立極地研究所)、中溝 葵(情報通信研究機構 電磁波計測研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、座長:野和田 基晴(山東大学)、座長:今城 峻(Kyushu Univ.)

16:15 〜 16:30

[PEM14-09] Conjugate Observations of Electromagnetic Ion Cyclotron (EMIC) Waves Associated with Traveling Convection Vortex (TCV) Events

*Hyomin Kim1C. Robert Clauer2Andrew Gerrard1Mark Engebretson3Michael Hartinger2Marc Lessard4Juergen Matzka5David Sibeck6Howard Singer7Claudia Stolle5Daniel Weimer2Zhonghua Xu2 (1.Center for Solar-Terrestrial Research, New Jersey Institute of Technology, USA、2.Center for Space Science and Engineering Research and Department of Electrical and Computer Engineering, Virginia Tech, USA、3.Department of Physics, Augsburg College, USA、4.Space Science Center, University of New Hampshire, USA、5.GFZ, German Research Centre for Geosciences, Germany、6.NASA Goddard Space Flight Center, USA、7.Space Weather Prediction Center, NOAA, USA)

キーワード:EMIC waves, Traveling Convection Vortex, Transient phenomena

We report on simultaneous observations of EMIC waves associated with traveling convection vortex (TCV) events caused by transient solar wind dynamic pressure (Pd) impulse events. The THEMIS spacecraft located near the magnetopause observed radial fluctuations of the magnetopause and the GOES spacecraft measured sudden compression of the magnetosphere in response to sudden increases in Pd. During the transient events, EMIC waves were observed by inter-hemispheric conjugate ground-based magnetometer arrays as well as the GOES spacecraft. The spectral structures of the waves appear to be well correlated with the fluctuating motion of the magnetopause, showing compression-associated wave generation. In addition, the wave features are remarkably similar in conjugate hemispheres in terms of bandwidth, periodic wave power modulation, and polarization. Proton precipitation was also observed by the DMSP spacecraft during the wave events, from which the wave source region is estimated to be 72-74 deg in magnetic latitude, consistent with the TCV center. The confluence of space-borne and ground instruments including the the inter-hemispheric, high-latitude, fluxgate/induction-coil magnetometer array allows us to constrain the EMIC source region while also confirming the relationship between EMIC waves and the TCV current system.