日本地球惑星科学連合2024年大会

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-EM11] Space Weather and Space Climate

2024年5月27日(月) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:片岡 龍峰(国立極地研究所)、Aronne Mary(NASA Goddard Space Flight Center)、伴場 由美(国立研究開発法人 情報通信研究機構)、Pulkkinen Antti(NASA Goddard Space Flight Center)

17:15 〜 18:45

[PEM11-P10] Statistical analysis of plasma energy flux distribution for spacecraft surface charging in the inner magnetosphere

*中村 雅夫1、松井 大智1 (1.大阪公立大学)

キーワード:宇宙機表面帯電、内部磁気圏、宇宙天気

Spacecraft surface charging is induced by the interaction of ambient plasma with the spacecraft surface and sometimes causes spacecraft anomalies due to electrostatic discharging (ESD) in the inner magnetosphere. We have studied surface charging events using data from the Electric Field and Wave (EFW) instruments and the Helium Oxygen Proton Electron (HOPE) sensors on the Van Allen Probes from 2012 to 2019. The results show that the surface charging events are distributed from the night side to the dawn side and the occurrence frequency of these events depends on solar activity. We statistically analyzed the plasma environment with a superposed analysis of the plasma energy flux distribution in the daylight region from the night side to the dawn side. The analysis reveals that a necessary condition for the negative surface charging is that the integral flux of high-energy (> 8 keV) electrons exceeds a threshold value and the total electron current is larger than the photoelectron current. A sufficient condition for the negative surface charging is that the low-energy electron flux is smaller than the flux observed during charging events because the current of secondary electrons generated by these low-energy electrons is smaller than the sum of all other currents. We will discuss the relationship between these charging conditions and space weather conditions.