Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science

Abstract A large magnetic storm occurred on October 10, 2024 and a super substorm occurred just after the shock arrival at 1520 UT. As a result, red auroras were photographed at multiple points over a wide region of Japan from 1700 UT (1 Japan local time). We apply a Bayesian analysis to estimate the time variation of the most probable height and latitude of the red aurora based on the citizen science data set, in combination with the POES/MetOp satellite data sets of electron precipitation boundary. We find that the top height of red aurora extended to ~ 950 km and the red aurora shifted toward low latitude according to the storm development. The ultra-high altitude of the red aurora can be evidence of rapid atmospheric heating and atmospheric expansion. Graphical abstract

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Publication Details

Journal
Earth Planets and Space
Published
2025-05-09
DOI
https://doi.org/10.1186/s40623-025-02178-w
Citations
5
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
5.77

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article

Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science

Shiori Uchino, S. A. Reddy, S. Nakano, Ryuho Kataoka
5 citations
Earth Planets and Space
Ionosphere and magnetosphere dynamics
5.77
article

Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science

Shiori Uchino, S. A. Reddy, S. Nakano, Ryuho Kataoka
article en
5 citations

Abstract

Abstract A large magnetic storm occurred on October 10, 2024 and a super substorm occurred just after the shock arrival at 1520 UT. As a result, red auroras were photographed at multiple points over a wide region of Japan from 1700 UT (1 Japan local time). We apply a Bayesian analysis to estimate the time variation of the most probable height and latitude of the red aurora based on the citizen science data set, in combination with the POES/MetOp satellite data sets of electron precipitation boundary. We find that the top height of red aurora extended to ~ 950 km and the red aurora shifted toward low latitude according to the storm development. The ultra-high altitude of the red aurora can be evidence of rapid atmospheric heating and atmospheric expansion. Graphical abstract

Earth Planets and SpaceVol. 77(1)
Okinawa Institute of Science and Technology Graduate University (JP), National Institute of Polar Research (JP), The Institute of Statistical Mathematics (JP), Research Organization of Information and Systems (JP)
Japan Society for the Promotion of Science
Openalex Percentile: Top 4%
Ionosphere and magnetosphere dynamics
5.77
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Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science — Shiori Uchino, S. A. Reddy, et al. · Earth Planets and Space (2025) | TGRS Research Map | TGRS