Whistler waves in the quasi-parallel and quasi-perpendicular magnetosheath
Ida Svenningsson, Emiliya Yordanova, Yuri V. Khotyaintsev, Mats, Andr\'e, Giulia Cozzani, Konrad Steinvall

TL;DR
This study statistically analyzes whistler waves in Earth's magnetosheath, revealing their occurrence, properties, and impact on electron pitch-angle scattering, with higher occurrence in quasi-perpendicular regions and significant effects on electron dynamics.
Contribution
It provides the first large-scale statistical characterization of whistler waves in the magnetosheath, quantifying their properties and role in electron scattering.
Findings
Higher whistler occurrence in quasi-perpendicular MSH
Whistler waves have median frequency of 0.2 times electron cyclotron frequency
Whistlers cause significant pitch-angle scattering of electrons
Abstract
In the Earth's magnetosheath (MSH), several processes contribute to energy dissipation and plasma heating, one of which is wave-particle interactions between whistler waves and electrons. However, the overall impact of whistlers on electron dynamics in the MSH remains to be quantified. We analyze 18 hours of burst-mode measurements from the Magnetospheric Multiscale (MMS) mission, including data from the unbiased magnetosheath campaign during February-March 2023. We present a statistical study of 34,409 whistler waves found using automatic detection. We compare wave occurrence in the different MSH geometries and find three times higher occurrence in the quasi-perpendicular MSH compared to the quasi-parallel case. We also study the wave properties and find that the waves propagate quasi-parallel to the background magnetic field, have a median frequency of 0.2 times the electron cyclotron…
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