Night-Side Relativistic Electron Precipitation Bursts in the Outer Radiation Belt: Insights from ELFIN and THEMIS

Fuente: arXiv
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Autores principales: Lu, Xi, Zhang, Xiao-Jia, Artemyev, Anton V., Angelopoulos, Vassilis, Bortnik, Jacob
Formato: Preprint
Publicado: 2024
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author Lu, Xi
Zhang, Xiao-Jia
Artemyev, Anton V.
Angelopoulos, Vassilis
Bortnik, Jacob
author_facet Lu, Xi
Zhang, Xiao-Jia
Artemyev, Anton V.
Angelopoulos, Vassilis
Bortnik, Jacob
contents Electromagnetic whistler-mode waves play a crucial role in the acceleration and precipitation of radiation belt electrons. Statistical surveys of wave characteristics suggest that these waves should preferentially scatter and precipitate relativistic electrons on the day side. However, the night-side region is expected to be primarily associated with electron acceleration. The recent low-altitude observations reveal relativistic electron precipitation in the night-side region. In this paper, we present statistical surveys of night-side relativistic electron losses due to intense precipitation bursts. We demonstrate that such bursts are associated with storm time substorm injections and are likely related to relativistic electron scattering by ducted whistler-mode waves. We also speculate on the role of injections in creating conditions favorable for relativistic electron precipitation.
format Preprint
id arxiv_https___arxiv_org_abs_2411_19232
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Night-Side Relativistic Electron Precipitation Bursts in the Outer Radiation Belt: Insights from ELFIN and THEMIS
Lu, Xi
Zhang, Xiao-Jia
Artemyev, Anton V.
Angelopoulos, Vassilis
Bortnik, Jacob
Space Physics
Plasma Physics
Electromagnetic whistler-mode waves play a crucial role in the acceleration and precipitation of radiation belt electrons. Statistical surveys of wave characteristics suggest that these waves should preferentially scatter and precipitate relativistic electrons on the day side. However, the night-side region is expected to be primarily associated with electron acceleration. The recent low-altitude observations reveal relativistic electron precipitation in the night-side region. In this paper, we present statistical surveys of night-side relativistic electron losses due to intense precipitation bursts. We demonstrate that such bursts are associated with storm time substorm injections and are likely related to relativistic electron scattering by ducted whistler-mode waves. We also speculate on the role of injections in creating conditions favorable for relativistic electron precipitation.
title Night-Side Relativistic Electron Precipitation Bursts in the Outer Radiation Belt: Insights from ELFIN and THEMIS
topic Space Physics
Plasma Physics
url https://arxiv.org/abs/2411.19232