Evidence of Electron Acceleration via Nonlinear Resonant Interactions with Whistler-mode Waves at Foreshock Transients

نویسندگان

چکیده

Abstract Shock waves are sites of intense plasma heating and charged particle acceleration. In collisionless solar wind plasmas, such acceleration is attributed to shock drift or Fermi but also wave–particle resonant interactions. We examine the latter for case electrons interacting with one most commonly observed wave modes in environments, whistler mode. Such particularly dynamic, localized regions upstream shocks, arising from kinetic interaction discontinuities. These regions, known as foreshock transients, significant electron by mechanisms not fully understood. Using situ observations transients Earth’s foreshock, we demonstrate that whistler-mode can resonate nonlinearly >25 eV accelerate them ∼100–500 eV. This mostly effective 50–250 energy range, where accelerated population exhibits a characteristic butterfly pitch-angle distribution consistent theoretical predictions. nonlinear very fast, implying this mechanism may be important injecting suprathermal origin into region, they undergo further, efficient shock-drift even higher energies.

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 2023

ISSN: ['2041-8213', '2041-8205']

DOI: https://doi.org/10.3847/1538-4357/acd9ab