[P-EM15] 太陽地球系結合過程の研究基盤形成

[PEM15-P03] Motion of the inverted-V structure during an isolated substorm

*田中 杜雄¹、田口 聡¹、高須 浩平¹、大井川 智一¹、細川 敬祐² (1.京都大学大学院理学研究科地球惑星科学専攻地球物理学教室、2.電気通信大学大学院情報理工学研究科)

キーワード：沿磁力線電流、オーロラ、inverted-V、isolated substorm

The inverted-V is an energetic electron precipitation event, which can be seen as a V-shape structure in electron flux spectrograms, and causes intense auroral arcs. Previous studies have suggested that the inverted-V structure can move fast poleward or equatorward. However, we still do not understand what drives its motion. In this study we have investigated the detailed characteristics of an inverted-V structure moving poleward, which occurred during an isolated substorm, using simultaneous observations of auroras, precipitating electrons, and field-aligned currents. We analyzed aurora data (630-nm and 557.7-nm) from an all-sky imager at Longyearbyen, Svalbard, and precipitating electrons and magnetic field data from the DMSP spacecraft (F16, F17, F18, F19). One of the interesting characteristics of the poleward-moving inverted-V is the appearance of a downward field-aligned current equatorward of and adjacent to the inverted-V. We discuss how the region of the downward field-aligned current evolves in association with the motion and growth/decay of the inverted V structure, and possibility of a role of the downward field-aligned current for the latitudinal motion of the inverted V.