講演情報
[PEM06-12]MMS satellites and EISCAT radar observations of dayside flow bursts.
*家田 章正1、小川 泰信2、大山 伸一郎1、北村 成寿3、斎藤 義文3、横田 勝一郎3、長谷川 洋3、田口 聡4、細川 敬祐5、町田 忍1、内野 宏俊4、堀 智昭1、Pollock C.6、Giles B.6、Moore T.6、Russell C.7、Strangeway R.7、中村 るみ8、Burch J.9 (1.名古屋大学 宇宙地球環境研究所、2.国立極地研究所、3.宇宙科学研究所、4.京都大学、5.電気通信大学、6.NASA Goddard Space Flight Center、7.University of California, Los Angeles、8.Space Research Institute, Austrian Academy of Sciences、9.Southwest Research Institute)
キーワード：
reconnection、MMS、EISCAT
A magnetic flux transfer event (FTE) was compared with ground radar observations of ionospheric ion flow bursts. Magnetospheric multiscale (MMS) satellites were located near the subsolar magnetopause at approximately 1049 UT on 15 December 2015. MMS satellites observed a southward turning of the interplanetary magnetic field (IMF), followed by a FTE 20 minutes later, and MMS entered the magnetosphere a further 10 minutes later. The European incoherent scatter (EISCAT) VHF radar at Tromso (Norway) was pointed to geographic north, with an elevation angle of 30 degrees, and was monitoring the ionospheric F region between 68 and 72 MLAT at 13 MLT. The Tromso radar did not observe an ionospheric flow burst at the time of the IMF southward turning but instead at the time of the FTE. A 630 nm all-sky imager at Longyearbean (74 MLAT, Norway) observed several poleward moving auroral forms (PMAFs) originating near 74 MLAT but none below 73 MLAT. The most significant PMAF accelerated and became enhanced approximately 3 minutes before the observation of the FTE. FTEs are usually associated with ionospheric flow bursts near the cusp and higher latitudes. In this particular case, it is suggested that the FTE is also associated with an ionospheric flow burst in subauroral latitudes. Such a subauroral flow burst may indicate a rarefaction inflow into the cusp and may occur when significant magnetic flux is removed by a FTE.