The dielectric response of plasmas with arbitrary gyrotropic velocity distributions

Hot and tenuous plasmas are frequently far from local thermodynamic equilibrium, necessitating sophisticated methods for determining the associated plasma dielectric tensor and normal mode response. The Arbitrary Linear Plasma Solver is a numerical tool for calculating such responses of plasmas with arbitrary gyrotropic background velocity distribution functions (VDFs). To model weakly and moderately damped plasma waves accurately, we have updated the code to use an improved analytic continuation enabled by a polynomial basis representation. We demonstrate the continuity of solutions to the linear Vlasov–Maxwell dispersion relation between bi-Maxwellian and arbitrary VDF representations and evaluate the influence of VDF structure on mode polarization and wave power emission and absorption.

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Publication Details

Journal
Physics of Plasmas
Published
2025-09-01
DOI
https://doi.org/10.1063/5.0286477
Citations
1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
1.15

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article

The dielectric response of plasmas with arbitrary gyrotropic velocity distributions

Daniel Verscharen, K. G. Klein
1 citations
Physics of Plasmas
Ionosphere and magnetosphere dynamics
1.15
article

The dielectric response of plasmas with arbitrary gyrotropic velocity distributions

Daniel Verscharen, K. G. Klein
article en
1 citations

Abstract

Hot and tenuous plasmas are frequently far from local thermodynamic equilibrium, necessitating sophisticated methods for determining the associated plasma dielectric tensor and normal mode response. The Arbitrary Linear Plasma Solver is a numerical tool for calculating such responses of plasmas with arbitrary gyrotropic background velocity distribution functions (VDFs). To model weakly and moderately damped plasma waves accurately, we have updated the code to use an improved analytic continuation enabled by a polynomial basis representation. We demonstrate the continuity of solutions to the linear Vlasov–Maxwell dispersion relation between bi-Maxwellian and arbitrary VDF representations and evaluate the influence of VDF structure on mode polarization and wave power emission and absorption.

Physics of PlasmasVol. 32(9)
Planetary Science Institute (US), University of Arizona (US), Department of Space (IN), University College London (GB)
National Science Foundation, National Aeronautics and Space Administration, Nuclear Safety and Security Commission, Science and Technology Facilities Council, Kavli Institute for Theoretical Physics, University of California, Santa Barbara, Heliophysics Division
Openalex Percentile: Top 17%
Ionosphere and magnetosphere dynamics
1.15
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