講演情報
[PEM13-P13]Time evolution of aurora structures associated with inverted-V electron distributions
*田中 杜雄1、田口 聡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、降下電子、inverted-V
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 satellite observations have suggested that the inverted-V structure would be stable for 5 min at least, but the detailed characteristics of its time evolution are still unclear. Aurora image data (557.7 nm and 630 nm) from an all-sky imager at Longyearbyen, Svalbard, and precipitating electron and magnetic field data from the DMSP spacecraft (F16, F17, F18, F19) are used to identify the aurora structures associated with inverted-V, and track their time evolution. The result of the analysis indicates that the auroral structures associated with inverted-V electron distributions tend to have longer durations than previously reported from the satellite observations. Some periodic features of the auroral structures are also seen. Key parameters for the stability of the inverted-V, i.e., parallel electric field are discussed in terms of phases of a substorm.