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  The Role of Local Acceleration and Radial Diffusion in Multi-MeV Electron Flux Enhancements

Saikin, A. A., Drozdov, A., Jaynes, A. N., Kondrashov, D., Boyd, A., Shprits, Y. (2025): The Role of Local Acceleration and Radial Diffusion in Multi-MeV Electron Flux Enhancements. - Journal of Geophysical Research: Space Physics, 130, 1, e2024JA033180.
https://doi.org/10.1029/2024JA033180

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Saikin, A. A.1, Author
Drozdov, A.2, Author              
Jaynes, A. N.1, Author
Kondrashov, D.1, Author
Boyd, A.1, Author
Shprits, Yuri3, Author              
Affiliations:
1External Organizations, ou_persistent22              
20 Pre-GFZ, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_146023              
31.5 Space Physics and Space Weather, 1.0 Geodesy, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum, ou_2239888              

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 Abstract: During the Van Allen Probes era, several multi-MeV (>4 MeV) electron flux enhancements were observed. The cause of electron acceleration up to multi-MeV remains an ongoing science topic. In this study, we focus on examining the relationship between phase space density (PSD) radial profile shapes and the occurrence of multi-MeV electron flux enhancement events. This will determine which process (local acceleration or radial diffusion) is dominant in producing multi-MeV electron flux enhancements at a specific L*. Growing peaks in PSD radial profiles are associated with the local acceleration (i.e., a wave-particle interaction) of multi-MeV electrons. For each growing peak in PSD, we determined the L* where the local acceleration occurs for each respective electron energy. Similarly, we also identify which PSD profiles are related to acceleration via radial diffusion profiles. Both sets of profiles are compared with the Van Allen Probe-A observed multi-MeV electron flux enhancements. Results show that both mechanisms (local acceleration and radial diffusion) can facilitate multi-MeV electron acceleration, however each mechanism has a preferable L* region where it is the dominant acceleration process.

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 Dates: 2025-01-262025
 Publication Status: Finally published
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 Identifiers: DOI: 10.1029/2024JA033180
GFZPOF: p4 T3 Restless Earth
OATYPE: Green Open Access
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Title: Journal of Geophysical Research: Space Physics
Source Genre: Journal, SCI, Scopus
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Pages: - Volume / Issue: 130 (1) Sequence Number: e2024JA033180 Start / End Page: - Identifier: ISSN: 2169-9380
ISSN: 2169-9402
CoNE: https://gfzpublic.gfz-potsdam.de/cone/journals/resource/jgr_space_physics
Publisher: Wiley
Publisher: American Geophysical Union (AGU)