日本地球惑星科学連合2016年大会

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インターナショナルセッション(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-EM09] Study of coupling processes in solar-terrestrial system

2016年5月23日(月) 15:30 〜 17:00 106 (1F)

コンビーナ:*山本 衛(京都大学生存圏研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、小川 泰信(国立極地研究所)、橋口 浩之(京都大学生存圏研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)、座長:小川 泰信(国立極地研究所)

16:05 〜 16:25

[PEM09-14] Significance of the D-region ion chemistry in the atmospheric forcing from above by precipitating high-energy particles

★招待講演

*Esa Turunen1 (1.Sodankyla Geophysical Observatory, University of Oulu)

キーワード:Ion chemistry, D region, aurora

Although the ionisation degree of middle atmosphere -lowere thermosphere region is low, it surprisingly turns out that ion chemistry plays a significant role in causing variations in concentrations of neutral chemically active minor constituents during events of excess ionisation, such as auroral particle precipitation. Here we first give an overview of the D-region ion chemistry, pointing out the relevant processes, which can be both direct and indirect via first generating chemically active minor constituents of the atmosphere, such as odd nitrogen and odd hydrogen, which in turn can affect for example atmospheric ozone via catalytic reactions either directly in-situ, or after transport in atmosphere to lower altitudes and lower latitudes. We show recent results using the detailed coupled neutral and ion chemistry model, the Sodankyla Ion Chemistry model. We also show how the upcoming new incoherent scatter radar facility EISCAT_3D, together with coordinated other currently planned measurements, will enhance the research opportunity in studying the coupling between geospace environment and atmosphere of Earth during high energy particle precipitation into the atmosphere.