Temperature anisotropy instabilities stimulated by the solar wind suprathermal populations

  • This review paper compiles recent results obtained by the present group of authors describing the effects of suprathermal populations present in space plasmas (up to a few keVs) on temperature anisotropy instabilities. Of particular interest are the electromagnetic cyclotron and firehose excitations, which play a major role in limiting temperature anisotropy, resulting, for instance, from the adiabatic expansion of the solar wind. Relying on a rigorous modeling and interpretation of the observed velocity distributions, both theoretical models and numerical simulations indicate a systematic stimulation of these excitations in the presence of suprathermal populations of electrons or protons. Moreover, the enhanced fluctuations react back on particles, and determine a faster and deeper relaxation of their anisotropy. The present comparative analysis suggests that previous studies, considering only quasi-thermal low-energy populations, may have significantly underestimated these excitations and their implications in various applications in space plasmas.

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Metadaten
Author:Marian LazarORCiDGND, Rodrigo LópezGND, Shaaban Mohammed ShaabanGND, Stefaan PoedtsGND, Peter Haesung YoonGND, Horst FichtnerORCiDGND
URN:urn:nbn:de:hbz:294-86797
DOI:https://doi.org/10.3389/fspas.2021.777559
Parent Title (English):Frontiers in astronomy and space sciences
Publisher:Frontiers Media
Place of publication:Lausanne
Document Type:Article
Language:English
Date of Publication (online):2022/03/04
Date of first Publication:2022/01/19
Publishing Institution:Ruhr-Universität Bochum, Universitätsbibliothek
Tag:instabilities; particle velocity distribution; solar wind; suprathermal particles; temperature
Volume:8
Issue:Article 777559
First Page:777559-1
Last Page:777559-12
Institutes/Facilities:Institut für Theoretische Physik IV
Dewey Decimal Classification:Naturwissenschaften und Mathematik / Physik
open_access (DINI-Set):open_access
faculties:Fakultät für Physik und Astronomie
Licence (English):License LogoCreative Commons - CC BY 4.0 - Attribution 4.0 International