Properties of Lower Hybrid Drift Waves and Energy Transfer Near and Inside the Magnetic Reconnection Electron Diffusion Regions

Abstract We investigate properties of lower hybrid drift waves (LHDWs) near and inside the electron diffusion regions in 17 magnetopause and 9 magnetotail reconnection events using Magnetospheric MultiScale (MMS) mission observations. Our analysis show that LHDW type depend on the electron beta, as electron beta increases LHDWs become more electromagnetic in nature. The energy transfer from electromagnetic fields to particles is higher in electrostatic LHDWs and it is largely in parallel direction with respect to the local magnetic field. Linear dispersion analysis shows that electrostatic LHDWs are perpendicular propagating while electromagnetic waves propagate in oblique directions and the normalized wavenumber of all LHDW types falls within 0.5–0.8 range. A simple estimate on the LHDW nonlinear saturation suggests a possibly important roles played by these waves in supporting the reconnection electric field.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2025-04-01
DOI
https://doi.org/10.1029/2024ja033238
Citations
4
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
4.62

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article

Properties of Lower Hybrid Drift Waves and Energy Transfer Near and Inside the Magnetic Reconnection Electron Diffusion Regions

A. K. Alex, R. E. Ergun, N. Ahmadi, Jongsoo Yoo et al.
4 citations
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
4.62
article

Properties of Lower Hybrid Drift Waves and Energy Transfer Near and Inside the Magnetic Reconnection Electron Diffusion Regions

A. K. Alex, R. E. Ergun, N. Ahmadi, Jongsoo Yoo, Rahul Banka, Hantao Ji, Emma Schultz‐Stachnik, Izzy Thomas
article en
4 citations

Abstract

Abstract We investigate properties of lower hybrid drift waves (LHDWs) near and inside the electron diffusion regions in 17 magnetopause and 9 magnetotail reconnection events using Magnetospheric MultiScale (MMS) mission observations. Our analysis show that LHDW type depend on the electron beta, as electron beta increases LHDWs become more electromagnetic in nature. The energy transfer from electromagnetic fields to particles is higher in electrostatic LHDWs and it is largely in parallel direction with respect to the local magnetic field. Linear dispersion analysis shows that electrostatic LHDWs are perpendicular propagating while electromagnetic waves propagate in oblique directions and the normalized wavenumber of all LHDW types falls within 0.5–0.8 range. A simple estimate on the LHDW nonlinear saturation suggests a possibly important roles played by these waves in supporting the reconnection electric field.

Journal of Geophysical Research Space PhysicsVol. 130(4)
University of Wisconsin–Parkside (US), University of Colorado Boulder (US), Princeton Plasma Physics Laboratory (US), Yale University (US), University of California San Diego (US), Laboratory for Atmospheric and Space Physics (US), Auburn University (US)
National Aeronautics and Space Administration, Heliophysics Division
Openalex Percentile: Top 6%
Ionosphere and magnetosphere dynamics
4.62
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Properties of Lower Hybrid Drift Waves and Energy Transfer Near and Inside the Magnetic Reconnection Electron Diffusion Regions — A. K. Alex, R. E. Ergun, et al. · Journal of Geophysical Research Space Physics (2025) | TGRS Research Map | TGRS