[P-EM12] Dynamics of the Inner Magnetospheric System

[PEM12-P24] A statistical study on high-energy electron injection events observed by Arase (ERG)

*楊 敬軒¹、篠原 育²、滑川 拓¹、三谷 烈史²、浅村 和史²、笠原 慧³、東尾 奈々⁴、松岡 彩子⁵ (1.東京大学 理学系研究科 地球惑星科学専攻、2.宇宙航空研究開発機構宇宙科学研究所、3.東京大学、4.宇宙航空研究開発機構、5.京都大学 理学研究科 地磁気世界資料解析センター)

The substorm injection is a critical phenomenon for supplying the free-energy necessary to generate relativistic electrons in the radiation belts. Numbers of studies on substorm injections have been demonstrated. However, how the injected electrons penetrate the inner magnetosphere and get their energy remains unclear. The energization of the particle injection is thought to be resulting from the transient enhancement of the electric field associated with the dipolarization, although there is no observational evidence such large electric fields accelerate injection particles.
Arase (ERG) often observes electron injections whose maximum energies reach hundreds of keV, while the typical maximum energy of injected electrons is about 100 keV or less. In this study, we would like to address how injected electrons are accelerated to such high energies. Collecting injection events during the period when the apogee of Arase is located in the nightside, we are examining the statistical properties of the high-energy injection events, e.g., the distribution of their estimated source regions, characteristics of energy spectra, pitch angle anisotropy, and other parameters in detail. We expect that finding dependence on the maximum energy is a key to limit the acceleration mechanisms of electron injections.
In the presentation, we will present preliminary results.