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-EM07] Dynamics in magnetosphere and ionosphere

2016年5月24日(火) 15:30 〜 17:00 103 (1F)

コンビーナ:*三好 由純(名古屋大学宇宙地球環境研究所)、田中 良昌(国立極地研究所)、中溝 葵(情報通信研究機構 電磁波計測研究所)、尾崎 光紀(金沢大学理工研究域電子情報学系)、中野 慎也(情報・システム研究機構 統計数理研究所)、堀 智昭(名古屋大学宇宙地球環境研究所)、座長:宮下 幸長(名古屋大学宇宙地球環境研究所)

16:00 〜 16:15

[PEM07-09] What if the evolution of auroral forms does not reflect magnetospheric processes?

*Shinichi Ohtani1 (1.The Johns Hopkins University Applied Physics Laboratory)

キーワード:Magnetosphere-ionosphere coupling, Aurora, Field-aligned currents

We often find auroral images very helpful for diagnosing magnetospheric processes, especially from a global point of view, supplementing spatially sparse satellite observations. The assumption that is very often made, if not explicitly, is that the temporal and spatial development of auroral forms reflects that of the corresponding magnetospheric processes. Although this assumption may be reasonable in many cases, caution needs to be exercised since the aurora is a manifestation of complex coupling between the magnetosphere and ionosphere, and the ionosphere does not always respond passively. In this presentation I shall discuss, with an actual example, how our perspective would change if the foundation of this assumption is not as solid as we generally consider.