arXiv Open Access 2024

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

Xi Lu Xiao-Jia Zhang Anton V. Artemyev Vassilis Angelopoulos Jacob Bortnik
Lihat Sumber

Abstrak

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.

Penulis (5)

X

Xi Lu

X

Xiao-Jia Zhang

A

Anton V. Artemyev

V

Vassilis Angelopoulos

J

Jacob Bortnik

Format Sitasi

Lu, X., Zhang, X., Artemyev, A.V., Angelopoulos, V., Bortnik, J. (2024). Night-Side Relativistic Electron Precipitation Bursts in the Outer Radiation Belt: Insights from ELFIN and THEMIS. https://arxiv.org/abs/2411.19232

Akses Cepat

Lihat di Sumber
Informasi Jurnal
Tahun Terbit
2024
Bahasa
en
Sumber Database
arXiv
Akses
Open Access ✓