Sub‐MeV Electron Precipitation Driven by EMIC Waves in Plasmaspheric Plumes at High <i>L</i> Shells

Abstract Electromagnetic ion cyclotron (EMIC) waves are known to be efficient for precipitating &gt;1 MeV electrons from the magnetosphere into the upper atmosphere. Despite considerable evidence showing that EMIC‐driven electron precipitation can extend down to sub‐MeV energies, the precise physical mechanism driving sub‐MeV electron precipitation remains an active area of investigation. In this study, we present an electron precipitation event observed by ELFIN CubeSats on 11 January 2022, exclusively at sub‐MeV energy at L ∼ 8–10.5, where trapped MeV electrons were nearly absent. The THEMIS satellites observed conjugate H‐band and He‐band EMIC waves and hiss waves in plasmaspheric plumes near the magnetic equator. Quasi‐linear diffusion results demonstrate that the observed He‐band EMIC waves, with a high ratio of plasma to electron cyclotron frequency, can drive electron precipitation down to ∼400 keV. Our findings suggest that exclusive sub‐MeV precipitation (without concurrent MeV precipitation) can be associated with EMIC waves, especially in the plume region at high L shells.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2025-03-01
DOI
https://doi.org/10.1029/2025ja033756
Citations
6
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
6.93

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article

Sub‐MeV Electron Precipitation Driven by EMIC Waves in Plasmaspheric Plumes at High L Shells

Qianli Ma, Wen Li, Murong Qin, Sheng Huang et al.
6 citations
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
6.93
article

Sub‐MeV Electron Precipitation Driven by EMIC Waves in Plasmaspheric Plumes at High L Shells

Qianli Ma, Wen Li, Murong Qin, Sheng Huang, Y. Nishimura, Xin An, Longzhi Gan, Luisa Capannolo, Anton Artemyev, Xiaochen Shen, V. Angelopoulos, Miroslav Hanzelka
article en
6 citations

Abstract

Abstract Electromagnetic ion cyclotron (EMIC) waves are known to be efficient for precipitating &gt;1 MeV electrons from the magnetosphere into the upper atmosphere. Despite considerable evidence showing that EMIC‐driven electron precipitation can extend down to sub‐MeV energies, the precise physical mechanism driving sub‐MeV electron precipitation remains an active area of investigation. In this study, we present an electron precipitation event observed by ELFIN CubeSats on 11 January 2022, exclusively at sub‐MeV energy at L ∼ 8–10.5, where trapped MeV electrons were nearly absent. The THEMIS satellites observed conjugate H‐band and He‐band EMIC waves and hiss waves in plasmaspheric plumes near the magnetic equator. Quasi‐linear diffusion results demonstrate that the observed He‐band EMIC waves, with a high ratio of plasma to electron cyclotron frequency, can drive electron precipitation down to ∼400 keV. Our findings suggest that exclusive sub‐MeV precipitation (without concurrent MeV precipitation) can be associated with EMIC waves, especially in the plume region at high L shells.

Journal of Geophysical Research Space PhysicsVol. 130(3)
Boston University (US), Planetary Science Institute (US), University of California, Los Angeles (US), Czech Academy of Sciences, Institute of Atmospheric Physics (CZ), GFZ Helmholtz Centre for Geosciences (DE)
National Science Foundation, National Aeronautics and Space Administration, Alexander von Humboldt-Stiftung, Nuclear Safety and Security Commission, Air Force Office of Scientific Research
Openalex Percentile: Top 4%
Ionosphere and magnetosphere dynamics
6.93
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