日本地球惑星科学連合2014年大会

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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-EM36_28PM2] 大気圏・電離圏

2014年4月28日(月) 16:15 〜 18:00 312 (3F)

コンビーナ:*大塚 雄一(名古屋大学太陽地球環境研究所)、津川 卓也(情報通信研究機構)、川村 誠治(独立行政法人 情報通信研究機構)、座長:松村 充(電気通信大学附属宇宙・電磁環境研究センター)、横山 竜宏(情報通信研究機構)

16:15 〜 16:30

[PEM36-22] 極冠パッチの縁

*細川 敬祐1田口 聡1小川 泰信2 (1.電気通信大学、2.国立極地研究所)

キーワード:極冠域電離圏, 大気光, 極冠パッチ, プラズマ不安定

A highly sensitive all-sky EMCCD airglow imager (ASI) has been operative in Longyearbyen, Norway (78.1N, 15.5E) since October 2011. One of the primary targets of this optical observation is a polar cap patch which is defined as an island of enhanced plasma density in the F region drifting anti-sunward across the central polar cap. Since the electron density within patches is often increased by a factor of 2?10 above that in the surrounding region, all-sky airglow measurements at 630.0 nm wavelength are capable of visualizing their spatial distribution in 2D fashion.During a 4-h interval on the night of December 4, 2013, a series of polar cap patches was observed by the ASI in Longyearbyen. By using the high-quality ASI images, we estimated the gradients in the leading/trailing edges of the patches and found that the gradient in the leading edge is 2-3 times steeper than that in the trailing edge. We also identified finger-like undulating structures growing along the trailing edge of the patches. Generation of these fingers is probably governed by a structuring through the gradient-drift instability which is known to occur only along one side of patches.From these observations, we suggest that such a structuring process can transport and mix the patch plasma across their trailing edges so that the scale size of the edges get extended. This means that the structuring through the plasma instability can strongly influence the large-scale shape of patches. Such a knowledge is of particular importance for better understanding the space weather effects of patches on the trans-ionospheric satellite communications in the polar cap region.