Relativistic Electron Precipitation Events Driven by Solar Wind Impact on the Earth's Magnetosphere

Roosnovo, Alexandra Katrina; Artemyev, Anton V.; Zhang, Xiao‐Jia; Angelopoulos, Vassilis; Ma, Qianli; Grimmich, Niklas; Plaschke, Ferdinand; Fischer, David; Werner, Magnes

doi:10.1029/2023ja032257

Title: Relativistic Electron Precipitation Events Driven by Solar Wind Impact on the Earth's Magnetosphere

Journal Article · 01 May 2024 · Journal of Geophysical Research. Space Physics

DOI: https://doi.org/10.1029/2023ja032257 · OSTI ID:2367508

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^[6]; Werner, Magnes ^[6]

Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
University of California, Los Angeles, CA (United States)
University of California, Los Angeles, CA (United States); University of Texas at Dallas, Richardson, TX (United States)
University of California, Los Angeles, CA (United States); Boston University, MA (United States)
Technische Universität Braunschweig, Braunschweig (Germany)
Austrian Academy of Science, Graz (Austria)

Certain forms of solar wind transients contain significant enhancements of dynamic pressure and may effectively drive magnetosphere dynamics, including substorms and storms. An integral element of such driving is the generation of a wide range of electromagnetic waves within the inner magnetosphere, either by compressionally heated plasma or by substorm plasma sheet injections. Consequently, solar wind transient impacts are traditionally associated with energetic electron scattering and losses into the atmosphere by electromagnetic waves. In this study, we show the first direct measurements of two such transient-driven precipitation events as measured by the low-altitude Electron Losses and Fields Investigation CubeSats. The first event demonstrates storm-time generated electromagnetic ion cyclotron waves efficiently precipitating sub-relativistic and relativistic electrons from >300 keV to 2 MeV at the duskside. The second event demonstrates whistler-mode waves leading to scattering of electrons from 50 to 700 keV on the dawnside. These observations confirm the importance of solar wind transients in driving energetic electron losses and subsequent dynamics in the ionosphere.

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Research Organization:: Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

Sponsoring Organization:: Air Force Office of Scientific Research (AFOSR); German Center for Aviation and Space (DLR); German Ministry for Economy and Technology; National Aeronautics and Space Administration (NASA); National Science Foundation (NSF); USDOE National Nuclear Security Administration (NNSA)

Grant/Contract Number:: 89233218CNA000001

OSTI ID:: 2367508

Report Number(s):: LA-UR-23-31472

Journal Information:: Journal of Geophysical Research. Space Physics, Journal Name: Journal of Geophysical Research. Space Physics Journal Issue: 5 Vol. 129; ISSN 2169-9380

Publisher:: American Geophysical UnionCopyright Statement

Country of Publication:: United States

Language:: English

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