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ALPS: The Arbitrary Linear Plasma Solver

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arxiv 1803.04697 v1 pith:I3VOI524 submitted 2018-03-13 physics.space-ph astro-ph.SRphysics.plasm-ph

classification physics.space-phastro-ph.SRphysics.plasm-ph
keywords alpsarbitraryplasmabackgrounddispersionnumericalparallelfield
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abstract

The Arbitrary Linear Plasma Solver (ALPS) is a parallelised numerical code that solves the dispersion relation in a hot (even relativistic) magnetised plasma with an arbitrary number of particle species with arbitrary gyrotropic equilibrium distribution functions for any direction of wave propagation with respect to the background field. ALPS reads the background momentum distributions as tables of values on a $(p_{\perp},p_{\parallel})$ grid, where $p_{\perp}$ and $p_{\parallel }$ are the momentum coordinates in the directions perpendicular and parallel to the background magnetic field, respectively. We present the mathematical and numerical approach used by ALPS and introduce our algorithms for the handling of poles and the analytic continuation for the Landau contour integral. We then show test calculations of dispersion relations for a selection of stable and unstable configurations in Maxwellian, bi-Maxwellian, $\kappa$-distributed, and J\"uttner-distributed plasmas. These tests demonstrate that ALPS derives reliable plasma dispersion relations. ALPS will make it possible to determine the properties of waves and instabilities in the non-equilibrium plasmas that are frequently found in space, laboratory experiments, and numerical simulations.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium

    physics.plasm-ph 2026-05 unverdicted novelty 7.0 of 10

    PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.

  2. The Dielectric Response of Plasmas with Arbitrary Gyrotropic Velocity Distributions

    physics.plasm-ph 2025-06 conditional novelty 6.0 of 10

    ALPS now uses high-order Chebyshev fits to improve the analytic continuation needed to compute damped plasma wave modes for arbitrary gyrotropic velocity distributions.

  3. Impact of Two-Population $\alpha$-particle Distributions on Plasma Stability

    astro-ph.SR 2024-12 conditional novelty 6.0 of 10

    Solar wind stability predictions match observed ion-scale wave signatures only when alpha particles are modeled as two populations (core and beam) rather than one.

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