JpGU-AGU Joint Meeting 2017

講演情報

[EE]Evening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-EM12] [EE] Space Weather, Space Climate, VarSITI

2017年5月23日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 7ホール)

[PEM12-P35] On two-dimensional distribution of trapped protons from solar cell degradation of the Akebono satellite

*三宅 亙1戸田 穂乃香1三好 由純2松岡 彩子3 (1.東海大学工学部、2.名古屋大学宇宙地球環境研究所、3.JAXA宇宙科学研究所)

キーワード:Akebono satellite, proton radiation belt, solar cell degradation

We have been studying on L-shell distribution of energetic (>10 MeV) protons from solar cell degradation of Akebono satellite orbiting in the inner magnetosphere. We obtained more compact distribution of the trapped protons than given by the AP8 and AP9 models. In our previous study (Miyake et al., 2014; 2015), we assumed that proton flux varies along the field line in the same rate as in the AP8 model. If the flux is more confined around the equator, the L-shell distribution may be possibly widen and the difference from the previous models can be smaller. Recent observation of the Van Allen probe has showed that quite anisotropic distribution of pitch angle which leads to spatial distribution confined near the equator (Selesnick et al., 2014). Thus, we introduce some different variation along the field line and seek the best-fit to the observed degradation of solar cells.