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-EM13] Dynamics of Magnetosphere and Ionosphere

コンビーナ:中溝 葵(情報通信研究機構 電磁波研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、藤本 晶子(九州工業大学)、佐藤 由佳(日本工業大学)

[PEM13-P02] Geomagnetic N+/O+ variation in the Ring Current Observed by the Arase (ERG) Satellite

*津田 洸一郎1横田 勝一郎1笠原 慧2桂華 邦裕3堀 智昭4三好 由純4篠原 育5寺田 健太郎1 (1.大阪大学院理学研究科宇宙地球科学専攻、2.東京大学、3.東京大学大学院理学系研究科地球惑星科学専攻、4.名古屋大学宇宙地球環境研究所、5.宇宙航空研究開発機構/宇宙科学研究所)

キーワード:Arase (ERG) 衛星、イオン流出、電離圏、窒素イオン

O+ and N+ are important ring current ions in magnetic storms and they can be a tracers of ion outflows from the deep ionosphere. Much Many researches haves been devoted to the escape of O+, but N+ has not been studied much, possibly because its mass per charge ratio is similar to that of O+ and separating the two is difficult.
We investigated the statistical properties of O+ and N+ in the ring current based on ion composition measurements (~10-180keV/q) by medium-energy particle experiments-ion mass analyzer (MEP-i) on board the Arase (Exploration of energization and Radiation in Geospace, ERG) satellite. By applying a fitting function to the TOF spectrum, we can separated N+ and O+ in the data obtained during geomagnetic storm on 16 July 2017. From the results of fitting we obtained the ratio of N+/O+. As a result the ratio of N+/O+ during geomagnetic storm and during geomagnetic quiet times is found to be about 0.2~0.4 and <0.2 respectively. In this presentation we will discuss ion outflow from the deep ionosphere.