Oblique Instability of Quasi-Parallel Whistler Waves in the Presence of Cold and Warm Electron Populations
Vadim Roytershteyn, Gian Luca Delzanno, Justin C. Holmes

TL;DR
This paper investigates the nonlinear instability of quasi-parallel whistler waves in Earth's magnetosphere, revealing how cold and warm electron populations influence oblique wave generation and plasma heating.
Contribution
It extends previous analysis by showing how low-energy electron distribution shapes the oblique whistler instability and demonstrates the instability's role in plasma heating and formation of resonant features.
Findings
Two distinct growth rate peaks associated with cold and warm electrons.
Oblique whistler instability persists even with high cold electron temperature.
Simulations show plasma heating and formation of resonant plateau and beam features.
Abstract
Whistler waves propagating nearly parallel to the ambient magnetic field experience a nonlinear instability that generates oblique electrostatic waves, including whistlers near the resonance cone that resemble oblique chorus in the Earth's magnetosphere. Focusing on the generation of oblique whistlers, earlier analysis of the instability is extended to the case where low-energy background plasma consists of both a "cold" population with energy ~ eV and a "warm" electron component with energy ~100 eV. This is motivated by observations in the Earth's magnetosphere where oblique chorus waves were shown to interact resonantly with the warm electrons. The main results are: i) the instability producing oblique whistlers is sensitive to the shape of the electron distribution at low energies. In the whistler range of frequencies, two distinct peaks in the growth rate are typically present: one…
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Taxonomy
TopicsOcean Waves and Remote Sensing · Oceanographic and Atmospheric Processes · Seismic Waves and Analysis
