Ion‐Acoustic Waves and the Proton‐Alpha Streaming Instability at Collisionless Shocks

Abstract Ion‐acoustic waves are routinely observed at collisionless shocks and could be an important source of resistivity. The source of instability and the effects of the waves are not fully understood. We show, using Magnetospheric Multiscale mission observations and numerical modeling, that across low Mach number shocks a large relative drift between protons and alpha particles develops, which can be unstable to the proton‐alpha streaming instability. Linear analysis and a numerical simulation show that the resulting waves agree with the observed wave properties. The generated ion‐acoustic waves are predicted to become nonlinear and form ion holes, maintained by trapped protons and alphas. The instability reduces the relative drift between protons and alphas, and heats the ions, thus providing a source of resistivity at shocks.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-05-03
DOI
https://doi.org/10.1029/2025gl115273
Citations
3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
3.46

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article

Ion‐Acoustic Waves and the Proton‐Alpha Streaming Instability at Collisionless Shocks

Ahmad Lalti, D. B. Graham, Y. V. Khotyaintsev
3 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
3.46
article

Ion‐Acoustic Waves and the Proton‐Alpha Streaming Instability at Collisionless Shocks

Ahmad Lalti, D. B. Graham, Y. V. Khotyaintsev
article en
3 citations

Abstract

Abstract Ion‐acoustic waves are routinely observed at collisionless shocks and could be an important source of resistivity. The source of instability and the effects of the waves are not fully understood. We show, using Magnetospheric Multiscale mission observations and numerical modeling, that across low Mach number shocks a large relative drift between protons and alpha particles develops, which can be unstable to the proton‐alpha streaming instability. Linear analysis and a numerical simulation show that the resulting waves agree with the observed wave properties. The generated ion‐acoustic waves are predicted to become nonlinear and form ion holes, maintained by trapped protons and alphas. The instability reduces the relative drift between protons and alphas, and heats the ions, thus providing a source of resistivity at shocks.

Geophysical Research LettersVol. 52(9)
Swedish Institute of Space Physics (SE), Northumbria University (GB)
Swedish National Space Agency, Knut och Alice Wallenbergs Stiftelse
Openalex Percentile: Top 8%
Ionosphere and magnetosphere dynamics
3.46
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Ion‐Acoustic Waves and the Proton‐Alpha Streaming Instability at Collisionless Shocks — Ahmad Lalti, D. B. Graham, et al. · Geophysical Research Letters (2025) | TGRS Research Map | TGRS