Whistler instabilities from the interplay of electron anisotropies in space plasmas: A quasilinear approach

TL;DR

This study uses a quasilinear approach to analyze how combined electron anisotropies and beaming populations drive whistler instabilities in space plasmas, revealing their interplay accelerates relaxation and thermalization processes.

Contribution

It provides a novel quasilinear analysis of the combined effects of electron anisotropies and beaming on whistler instabilities, bridging gaps between separate studies.

Findings

Cumulative effects enhance whistler fluctuations.

Faster relaxation of beaming velocity and electron thermalization.

Explanation for observed near-isotropic electron states.

Abstract

Recent statistical studies of observational data unveil relevant correlations between whistler fluctuations and the anisotropic electron populations present in space plasmas, e.g., solar wind and planetary magnetospheres. Locally, whistlers can be excited by two sources of free energy associated with anisotropic electrons, i.e., temperature anisotropies and beaming populations carrying the heat flux. However, these two sources of free energy and the resulting instabilities are usually studied independently preventing a realistic interpretation of their interplay. This paper presents the results of a parametric quasilinear study of the whistler instability cumulatively driven by two counter-drifting electron populations and their anisotropic temperatures. By comparison to individual regimes dominated either by beaming population or by temperature anisotropy, in a transitory regime the instability becomes highly conditioned by the effects of both these two sources of free energy. Cumulative effects stimulate the instability and enhance the resulting fluctuations, which interact with electrons and stimulate their diffusion in velocity space, leading to a faster and deeper relaxation of the beaming velocity associated with a core heating in perpendicular direction and a thermalization of the beaming electrons. In particular, the relaxation of temperature anisotropy to quasi-stable states below the thresholds conditions predicted by linear theory may explain the observations showing the accumulation of these states near the isotropy and equipartition of energy.