High temporal- and spatial-resolution photographs of the “Christmas” red-green auroras taken over Germany during a main phase of the 10–11 May 2024 superstorm

Abstract. High spatial and temporal resolution images of red auroras over Germany during the 10–11 May 2024 magnetic storm have added new information concerning stable auroral red (SAR) arc formation. The high-altitude red aurora displayed brightness streaks/rays, which continued to lower altitude green auroral brightness rays, indicating that energetic electron precipitation along the Earth’s magnetic field lines are causing both auroras. Both the red and green auroras are diffuse in nature, indicating that instability of high-energy ring current particles inside the plasmasphere followed by wave-particle interactions is the most likely cause of the precipitating electrons. The 5577Å diffuse green aurora below the SAR arcs is a new scientific finding. This is named Stable Auroral Green (SAG) arcs. The SAR and SAG arc images were taken during the first and second steps of the 2024 superstorm. They occurred during intense substorms.

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Publication Details

Journal
Annales Geophysicae
Published
2026-11-03
DOI
https://doi.org/10.5194/angeo-44-1201-2026
Citations
1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
2.43

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article

High temporal- and spatial-resolution photographs of the “Christmas” red-green auroras taken over Germany during a main phase of the 10–11 May 2024 superstorm

Richard Bertram Horne, Klaus Reinsch, Ingo von Borstel, Yasuhito Narita et al.
1 citations
Annales Geophysicae
Ionosphere and magnetosphere dynamics
2.43
article

High temporal- and spatial-resolution photographs of the “Christmas” red-green auroras taken over Germany during a main phase of the 10–11 May 2024 superstorm

Richard Bertram Horne, Klaus Reinsch, Ingo von Borstel, Yasuhito Narita, Gurbax Singh Lakhina, Rajkumar Hajra, Sami Khan Solanki, V. Bothmer, Bruce Tsatnam Tsurutani, Masatomi Iizawa, Karl-Heinz Glassmeier
article en
1 citations

Abstract

Abstract. High spatial and temporal resolution images of red auroras over Germany during the 10–11 May 2024 magnetic storm have added new information concerning stable auroral red (SAR) arc formation. The high-altitude red aurora displayed brightness streaks/rays, which continued to lower altitude green auroral brightness rays, indicating that energetic electron precipitation along the Earth’s magnetic field lines are causing both auroras. Both the red and green auroras are diffuse in nature, indicating that instability of high-energy ring current particles inside the plasmasphere followed by wave-particle interactions is the most likely cause of the precipitating electrons. The 5577Å diffuse green aurora below the SAR arcs is a new scientific finding. This is named Stable Auroral Green (SAG) arcs. The SAR and SAG arc images were taken during the first and second steps of the 2024 superstorm. They occurred during intense substorms.

Annales GeophysicaeVol. 44(2)
University of Science and Technology of China (CN), British Antarctic Survey (GB), Jet Propulsion Laboratory (US), Indian Navy (IN), Kyung Hee University (KR), Max Planck Institute for Solar System Research (DE), Fraunhofer Institute for Surface Engineering and Thin Films (DE), Indian Institute of Geomagnetism (IN), University of Göttingen (DE), Technische Universität Braunschweig (DE)
National Natural Science Foundation of China, Chinese Academy of Sciences, Young Scientists Fund
Openalex Percentile: Top 16%
Ionosphere and magnetosphere dynamics
2.43
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