Stability and Characteristics of Lower-hybrid Drift Waves: Dependence on Electron Beta and Cross-field Relative Drift

Abstract Lower-hybrid drift waves (LHDWs) are frequently observed microinstabilities in both space and laboratory plasmas. Despite decades of study, the relationship between electrostatic (ES-LHDW) and electromagnetic (EM-LHDW) variants and the plasma parameters controlling their stability remains unclear. Here, we systematically examine LHDW behavior by solving the local linear dispersion relation over a wide range of plasma and field conditions. Our results demonstrate that ES-LHDWs and EM-LHDWs are not distinct modes but rather two different regimes of the same drift wave whose character evolves smoothly with electron beta ( β e ) and the cross-field electron drift velocity relative to ions, normalized to the ion sound speed ( u 0 x / C s ). The nature of the waves changes from electrostatic to electromagnetic when β e increases. Growth rates increase with u 0 x / C s but decrease with β e , while the most unstable wavelength remains nearly universal, with kρ e ∼ 0.8 ( k is the magnitude of the wave vector and ρ e is the electron gyroradius). We further present quasi-linear estimates of nonlinear saturation properties, including energy partition among electric fields, magnetic fields, and particle kinetic responses. We show that ES-LHDWs reach higher electric-field saturation amplitudes, whereas EM-LHDWs generate strong magnetic perturbations and parallel electric fields that may enable efficient particle heating. Comparisons with the classical model reveal that retaining electromagnetic effects is essential for accurate predictions of frequency, growth rate, and the propagation angle. These findings provide a unified framework for understanding LHDWs across diverse collisionless plasma environments, including current sheets of magnetic reconnection, shear layers, collisionless shocks, and boundary regions.

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Publication Details

Journal
The Astrophysical Journal
Published
2026-03-26
DOI
https://doi.org/10.3847/1538-4357/ae4ec0
Primary Topic
Magnetic confinement fusion research
Type
article
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article

Stability and Characteristics of Lower-hybrid Drift Waves: Dependence on Electron Beta and Cross-field Relative Drift

Peiyun Shi, A.B. Robbins, Kush Maheshwari, Euichan Jung et al.
The Astrophysical Journal
Magnetic confinement fusion research
article

Stability and Characteristics of Lower-hybrid Drift Waves: Dependence on Electron Beta and Cross-field Relative Drift

Peiyun Shi, A.B. Robbins, Kush Maheshwari, Euichan Jung, Jonathan Ng, Sayak Bose, Li-Jen Chen, Hantao Ji, Jongsoo Yoo
article en

Abstract

Abstract Lower-hybrid drift waves (LHDWs) are frequently observed microinstabilities in both space and laboratory plasmas. Despite decades of study, the relationship between electrostatic (ES-LHDW) and electromagnetic (EM-LHDW) variants and the plasma parameters controlling their stability remains unclear. Here, we systematically examine LHDW behavior by solving the local linear dispersion relation over a wide range of plasma and field conditions. Our results demonstrate that ES-LHDWs and EM-LHDWs are not distinct modes but rather two different regimes of the same drift wave whose character evolves smoothly with electron beta ( β e ) and the cross-field electron drift velocity relative to ions, normalized to the ion sound speed ( u 0 x / C s ). The nature of the waves changes from electrostatic to electromagnetic when β e increases. Growth rates increase with u 0 x / C s but decrease with β e , while the most unstable wavelength remains nearly universal, with kρ e ∼ 0.8 ( k is the magnitude of the wave vector and ρ e is the electron gyroradius). We further present quasi-linear estimates of nonlinear saturation properties, including energy partition among electric fields, magnetic fields, and particle kinetic responses. We show that ES-LHDWs reach higher electric-field saturation amplitudes, whereas EM-LHDWs generate strong magnetic perturbations and parallel electric fields that may enable efficient particle heating. Comparisons with the classical model reveal that retaining electromagnetic effects is essential for accurate predictions of frequency, growth rate, and the propagation angle. These findings provide a unified framework for understanding LHDWs across diverse collisionless plasma environments, including current sheets of magnetic reconnection, shear layers, collisionless shocks, and boundary regions.

The Astrophysical JournalVol. 1000(2)
Goddard Space Flight Center (US), Princeton University (US), Princeton Plasma Physics Laboratory (US), Institute of Astronomy (RU), University of Maryland, College Park (US)
Openalex Percentile: Top 7%
Magnetic confinement fusion research
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