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-P12] Improvement of detector response matrices of the high-energy electron experiments (HEP) onboard the Arase satellite

*三谷 烈史1PARK INCHUN2堀 智昭2高島 健1笠原 慧3栗田 怜2寺本 万里子4東尾 奈々1三好 由純2篠原 育1 (1.宇宙航空研究開発機構、2.名古屋大学、3.東京大学、4.九州工業大学)

キーワード:あらせ衛星、高エネルギー電子

The high-energy electron experiments (HEP) onboard the Arase satellite detects 70 keV-2 MeV electrons and generates three-dimensional velocity distribution data for these electrons in every period of the satellite's rotation. Electrons are detected by two instruments, HEP-L and HEP-H, which differ in their geometric factor (G-factor) and energy range they cover. HEP-L detects 70 keV–1 MeV electrons with the G-factor of 9.3 × 10−4 cm2 sr at maximum, while HEP-H observes 0.7 MeV–2 MeV electrons with the G-factor of 9.3 × 10-3 cm2 sr at maximum. The instruments utilize silicon strip detectors and application-specific integrated circuits to read out incident charge signals from each strip.

In order to deduce the distribution of incident electrons from the direction and energy detections in orbit, we have developed a detector simulator using the Geant4 toolkit. Using the simulator, we calculate response matrices of the detectors and derive incident fluxes from the detected counts. The derived fluxes of electrons at around 100 keV are consistent with those observed by the medium-energy particle experiments - electron analyzer (MEP-e), which utilizes an electrostatic analyzer.

Recently, we have evaluated effects on detection efficiency caused by on-board signal processing. We found that the detection efficiency for higher energy electrons affected by parameters such as an energy threshold and readout noise, which are used to determine whether to read out the signal from the detector. We have updated the response matrices taking those parameters into account. In this presentation, we will present our calibration methods and their evaluation status. Especially, we will show a comparison before and after updating the matrices.