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Magnetic storm-time red aurora as seen from Hokkaido, Japan on December 1, 2023 associated with high-density solar wind
  • +4
  • Ryuho Kataoka,
  • Yoshizumi Miyoshi,
  • Kazuo Shiokawa,
  • Nozomu Nishitani,
  • Kunihiro Keika,
  • Takanobu AMANO,
  • Kanako Seki
Ryuho Kataoka
National Institute of Polar Research

Corresponding Author:[email protected]

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Yoshizumi Miyoshi
Institute for Space-Earth Environmental Research, Nagoya University
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Kazuo Shiokawa
Institute for Space-Earth Environmental Research, Nagoya University
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Nozomu Nishitani
Nagoya University, Japan
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Kunihiro Keika
The University of Tokyo
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Takanobu AMANO
University of Tokyo
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Kanako Seki
The University of Tokyo
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Abstract

We report a citizen science-motivated study on the cause of an unusually bright red aurora as witnessed from Hokkaido, Japan during a magnetic storm on December 1, 2023. Such an intense red aurora event has occurred in the Halloween 2003 super storm, but the Dst index peak of this December 2023 storm was only -107 nT. In spite of the moderate storm amplitude, the extremely high solar wind density of >50 /cc caused the aurora oval extension to 53 MLAT (L=2.8). We discuss that the drift loss of the ring current particles across the small-size magnetopause is important, and Hokkaido was at the right position to see the direct effect of the large particle injection of the storm-time substorm.
21 Feb 2024Submitted to ESS Open Archive
28 Feb 2024Published in ESS Open Archive