pith:KSWSJR4W
Resonant shear-flow instability in anisotropic supersonic plasmas with heat flux
A resonant instability develops in supersonic shear flows of anisotropic collisionless plasmas and disappears in the vortex sheet limit.
arxiv:2605.13056 v1 · 2026-05-13 · astro-ph.SR · physics.plasm-ph
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Claims
The instability is identified as resonant, peaking when the wave phase velocity matches the mean flow velocity, with the growth rate decreasing for higher-order modes... the instability vanishes in the vortex sheet limit, distinguishing it from the classical Kelvin-Helmholtz mechanism. These findings suggest that this specific instability holds significant potential for explaining the problem of observed boundaries between isotropic and anisotropic proton temperature regions in a low-beta solar wind plasma.
The reduction of the governing wave equation to an exactly solvable form assumes a smooth hyperbolic velocity profile together with spatially homogeneous density and magnetic field in the unperturbed state; the 16-moment closure must remain valid throughout the linear growth phase.
An exact analytical modal analysis yields a resonant shear-flow instability in supersonic anisotropic plasmas that vanishes in the vortex-sheet limit and is distinct from Kelvin-Helmholtz.
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| First computed | 2026-05-18T03:08:59.196271Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
54ad24c796bb1a662a3ea341f170ffe6c900c0cd50931f5d7b19636d1bec2a6c
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/KSWSJR4WXMNGMKR6UNA7C4H743 \
| jq -c '.canonical_record' \
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Canonical record JSON
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