宇宙空間のプラズマ波動の源を可視化する「リング状に拡大する脈動オーロラ」を世界で初めて発見

20206-06-17 電気通信大学

電気通信大学、名古屋大学、国立極地研究所、京都大学などの国際共同研究グループは、北欧フィンランドのソダンキュラに設置された高速EMCCD全天カメラと、地球磁気圏探査衛星「あらせ(ERG)」の同時観測により、世界で初めて「リング状に急速拡大する脈動オーロラ」を発見した。観測では、パッチ状オーロラがわずか約10秒の間に全方位へ拡大し、中心部に暗い領域(ダークホール)を持つリング状構造へ変化する様子を捉えた。衛星観測では同時に自然のプラズマ波動である「コーラス波」の強度上昇が検出され、オーロラの拡大と数秒の時間差で対応していた。この結果から、リング状オーロラはコーラス波の発生源(波源領域)そのものが宇宙空間で急速に拡大したことを可視化した現象であることが判明した。さらに研究チームは、その拡大要因として速進磁気音波(ファストモード波)の関与を提案している。本成果は、地上から観測されるオーロラを利用して宇宙空間のプラズマ波動や放射線帯電子のダイナミクスを遠隔可視化できる可能性を示し、地球のみならず木星など他惑星のオーロラ研究にも新たな展開をもたらすものである。

宇宙空間のプラズマ波動の源を可視化する「リング状に拡大する脈動オーロラ」を世界で初めて発見
図2:500ミリ秒毎に取得されたオーロラの連続画像。パッチ状のオーロラが出現し、円弧状に拡大しながら、最終的にはリング状の構造になる様子を示しています。

<関連情報>

円形に膨張するリング状の脈動オーロラ:宇宙におけるプラズマ波源の可視化 Circularly Expanding Ring-Shaped Pulsating Aurora Visualizing the Source of Plasma Waves in Space

K. Hosokawa, S. Kurita, Y. Miyoshi, S.-I. Oyama, Y. Ogawa, M. Ozaki, Y. Kasahara, Y. Kasaba, S. Yagitani, S. Matsuda, F. Tsuchiya, A. Kumamoto, A. Matsuoka, S. Imajo, T. Raita, E. Turunen,…
AGU Advances  Published: 04 June 2026
DOI:https://doi.org/10.1029/2026AV002300

Abstract

Pulsating aurorae are prominent auroral emissions in the polar regions, typically occurring in the morning hours during the recovery phase of auroral substorms. These aurorae usually consist of round-shaped patches of emission, with luminosity that pulsates at intervals ranging from less than a second to several tens of seconds. Here, we present, for the first time, a unique case of a pulsating aurora that expanded radially outward in all the directions and repeatedly formed a ring-shaped structure. The speed of expansion, which was at least several tens of kilometers per second at ionospheric altitudes, cannot be attributed to the horizontal convective motion of plasma in the ionosphere. In the magnetosphere, corresponding to the expanding ring-shaped aurora, the Arase satellite detected successive enhancements of natural electromagnetic waves known as a “chorus.” These chorus waves scatter energetic magnetospheric electrons into the ionosphere, resulting in pulsating diffuse aurorae. Notably, the satellite observed systematic delay in the timing of chorus detections, which suggests that a similar circularly expanding feature existed in space. These simultaneous observations of expanding features in both the ionosphere and the magnetosphere demonstrate that the temporal evolution of the shape of a pulsating aurora manifests the spatiotemporal evolution of the source of plasma waves in space.

Plain Language Summary

Pulsating aurorae are faint, patchy auroral lights that repeatedly turn on and off over polar regions, usually after geomagnetic disturbances. Although their time variations have been studied extensively, how their shapes change in space has remained unclear. Here, we report a unique pulsating aurora that formed a thin ring and expanded rapidly outward in all directions within only a few seconds. This unusual aurora was captured using a high-speed all-sky camera in northern Finland, allowing us to observe its detailed evolution for the first time. At the same time, the Arase satellite observed electromagnetic plasma waves, called chorus waves, in Earth’s magnetosphere. These waves are known to scatter energetic electrons into the atmosphere, producing pulsating aurorae. We found that the chorus waves detected by the satellite appeared with systematic time delays that matched the outward expansion of the auroral ring seen from the ground. This indicates that the source region of the chorus waves in space was itself expanding. Our results suggest that disturbances in the magnetosphere can spread rapidly through plasma waves and directly control the shapes of aurorae observed in the upper atmosphere. This study demonstrates that auroral imaging can be used as a remote tool to visualize dynamic plasma processes occurring more than tens of thousands of kilometers above Earth.

1702地球物理及び地球化学
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