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.
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Kataoka, R., Nakano, S., Uchino, S., & Reddy, S. A. (2025, December 1). Extended red aurora associated with super substorm igniting the October 10, 2024 magnetic storm as revealed by citizen science. Earth, Planets and Space. Springer Science and Business Media Deutschland GmbH. https://doi.org/10.1186/s40623-025-02178-w
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