JpGU-AGU Joint Meeting 2020

講演情報

[E] ポスター発表

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-EM19] Dynamics of the Inner Magnetospheric System

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、三好 由純(名古屋大学宇宙地球環境研究所)、Lynn M Kistler(University of New Hampshire Main Campus)

[PEM19-P13] Inter-channel normalization and energy spectrum correction of the high-energy electron experiments (HEP) onboard the Arase satellite

*堀 智昭1三谷 烈史2高島 健2Park InChun1栗田 怜1寺本 万里子3東尾 奈々4笠原 慧5横田 勝一郎6三好 由純1篠原 育2 (1.名古屋大学宇宙地球環境研究所、2.宇宙科学研究所、3.九州工業大学、4.宇宙航空研究開発機構、5.東京大学、6.大阪大学)

Detailed evaluation of the relative efficiency of azimuthal channels and their dependence on the energy of incident electrons has been conducted for the high-energy electron experiments (HEP) onboard the Arase satellite since the start of the satellite operation. Recently the simulation model of the instrument response has been improved to consider a realistic threshold and noise level of the onboard electronics for triggering an event of electron incidence in the detector system. The updated simulation model brings out new response properties of the instrument which could significantly modify the incident energy dependence as well as the relative efficiency among azimuthal channels, particularly at high energy. Accordingly, science data products such as Level-2 electron differential flux data are also to be updated on the basis of newly deduced calibration parameters. We show how the new electron flux data and their angular distribution are compared to the previous versions. Comparison with flux data of the other electron instruments onboard shows the same level of consistency in flux value for the lower energy part, while there still remains some discrepancy in the MeV range.