日本地球惑星科学連合2022年大会

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[E] 口頭発表

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-EM10] Dynamics of Magnetosphere and Ionosphere

2022年5月26日(木) 15:30 〜 17:00 303 (幕張メッセ国際会議場)

コンビーナ:佐藤 由佳(日本工業大学)、コンビーナ:家田 章正(名古屋大学 宇宙地球環境研究所)、藤本 晶子(九州工業大学)、コンビーナ:今城 峻(京都大学大学院理学研究科附属地磁気世界資料解析センター)、座長:田中 良昌(国立極地研究所)、北村 成寿(東京大学大学院 理学系研究科 地球惑星科学専攻)


15:30 〜 15:45

[PEM10-17] Curved Trajectory Effect on Charge-Exchange Collision at Ionospheric Temperatures

*家田 章正1 (1.名古屋大学 宇宙地球環境研究所)

キーワード:電荷交換衝突、分極衝突、衝突周波数、断面積、電子移行、運動量輸送

Collision between ions and neutral particles is an essential characteristic of Earth's ionosphere. This ion-neutral collision is usually caused by the polarization of neutral particles. This collision can also be caused by charge exchange, if the particle pair is parental, such as atomic oxygen and its ion. The total collision frequency is not the sum of the polarization and charge-exchange components, but is essentially equal to the dominant component. The total is enhanced only around the classic transition temperature, which is near the ionospheric temperature range (typically 200–2000 K). However, the magnitude of this enhancement has differed among previous studies; the maximum enhancement has been reported as 41% and 11% without physical explanation. In the present study, the contribution of the polarization force to the charge-exchange collision is expressed as a simple curved particle trajectory effect. As a result, the maximum enhancement is found to be 22%. It is discussed that the enhancement has been neglected in classic ionospheric studies partly due to confusion with the glancing particle contribution, which adds 10.5% to the polarization component. The enhancement has been neglected presumably also because there has been no functional form to express it. Such an expression is derived in this study.

Ieda (JGR, 2022) https://doi.org/10.1029/2021JA029612