Exceptionally gigantic aurora in the polar cap on a day when the solar wind almost disappeared

Author:

Hosokawa Keisuke12ORCID,Kataoka Ryuho3,Tsuda Takuo T.12,Ogawa Yasunobu3ORCID,Taguchi Satoshi4ORCID,Zhang Yongliang5ORCID,Paxton Larry J.5ORCID

Affiliation:

1. Graduate School of Communication Engineering and Informatics, University of Electro-Communications, Tokyo 182-8585, Japan.

2. Center for Space Science and Radio Engineering, University of Electro-Communications, Tokyo 182-8585, Japan.

3. National Institute of Polar Research, Tokyo 190-0014, Japan.

4. Graduate School of Science, Kyoto University, Kyoto 606-8502, Japan.

5. The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA.

Abstract

Revealing the origins of aurorae in Earth’s polar cap has long been a challenge since direct precipitation of energetic electrons from the magnetosphere is not always expected in this region of open magnetic field lines. Here, we introduce an exceptionally gigantic aurora filling the entire polar cap region on a day when the solar wind had almost disappeared. By combining ground-based and satellite observations, we proved that this unique aurora was produced by suprathermal electrons streaming directly from the Sun, which is known as “polar rain.” High-sensitivity imaging from the ground has visualized complex spatial structures of the polar rain aurora possibly manifesting the internal pattern of the solar wind or even the organizations in the chromosphere of the Sun.

Publisher

American Association for the Advancement of Science (AAAS)

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