Magnetic Storm‐Time Red Aurora as Seen From Hokkaido, Japan on 1 December 2023 Associated With High‐Density Solar Wind

• Published in: Geophysical research letters 2024-06, Vol.51 (12), p.n/a
• Main Authors: Kataoka, Ryuho, Miyoshi, Yoshizumi, Shiokawa, Kazuo, Nishitani, Nozomu, Keika, Kunihiro, Amano, Takanobu, Seki, Kanako
• Format: Article
• Language: English
• Subjects: aurora; Auroras; citizen science; Density; DST Index; Dynamic pressure; Geomagnetic storms; interplanetary shock; magnetic storm; Magnetic storms; Magnetopause; Particle injection; Particle size; Ring currents; Solar wind; Solar wind density; Storm effects; Storms
• ISSN: 0094-8276; 1944-8007
• DOI: 10.1029/2024GL108778

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 1 December 2023. The auroral brightness of 5 kR is unusual for the Dst index peak of only −107 nT. In spite of the moderate storm amplitude, the extremely high solar wind density of >50/cc and dynamic pressure of >25 nPa caused the aurora oval extension to 53 magnetic latitudes (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. Plain Language Summary Citizen scientists identified an unusually bright red aurora from Hokkaido, Japan during a not‐so‐unusual magnetic storm on 1 December 2023. The large dynamic pressure, driven by large density of >50/cc, contributed to a small magnetopause and the effects observed at such low latitude. The hypothesis of this study is that the loss of ring current particles across the small‐size magnetopause played an important role. Also, we discuss that Hokkaido was at the right position to see the direct effect of storm‐time substorm. Key Points Unusually bright red aurora was witnessed by citizen scientists from Hokkaido, Japan on 1 December 2023 The magnetic storm amplitude was not unusually large, but the solar wind density was high (50/cc) Dynamic pressure and asymmetric evolution of the ring current are important to understand the cause of red‐aurora magnetic storm events