O‐Mode Instability for Non‐Thermal Continuum Radiation Generated Near the Plasmapause

Abstract Analysis of the ordinary mode (O‐mode) instability is performed to comprehend the nonthermal continuum (NTC) radiation near the plasmapause, taking into account the relativistic wave‐electron resonance effect. The energy source is the anisotropy in the velocity of the minority suprathermal electron population. Numerical solutions demonstrate that the O‐mode can be unstable with multiple narrow frequency bands located close to harmonics of the electron cyclotron frequency above the local electron plasma frequency. These waves have narrow beaming angle bands of nearly relative to the ambient magnetic field. Our findings indicate that NTC radiation generated by this wave‐electron resonance instability near the plasmapause can propagate nearer to the magnetic equator with multiple harmonics, which is in agreement with a recent statistical study using Van Allen Probes.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2024-10-01
DOI
https://doi.org/10.1029/2024ja032626
Citations
1
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.33

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article

O‐Mode Instability for Non‐Thermal Continuum Radiation Generated Near the Plasmapause

S. A. Boardsen, Iver H. Cairns, J. R. Johnson, C. Z. Cheng et al.
1 citations
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
0.33
article

O‐Mode Instability for Non‐Thermal Continuum Radiation Generated Near the Plasmapause

S. A. Boardsen, Iver H. Cairns, J. R. Johnson, C. Z. Cheng, Eun‐Hwa Kim
article en
1 citations

Abstract

Abstract Analysis of the ordinary mode (O‐mode) instability is performed to comprehend the nonthermal continuum (NTC) radiation near the plasmapause, taking into account the relativistic wave‐electron resonance effect. The energy source is the anisotropy in the velocity of the minority suprathermal electron population. Numerical solutions demonstrate that the O‐mode can be unstable with multiple narrow frequency bands located close to harmonics of the electron cyclotron frequency above the local electron plasma frequency. These waves have narrow beaming angle bands of nearly relative to the ambient magnetic field. Our findings indicate that NTC radiation generated by this wave‐electron resonance instability near the plasmapause can propagate nearer to the magnetic equator with multiple harmonics, which is in agreement with a recent statistical study using Van Allen Probes.

Journal of Geophysical Research Space PhysicsVol. 129(10)
Andrews University (US), University of Maryland, Baltimore (US), The University of Sydney (AU), Goddard Space Flight Center (US), Princeton University (US), Princeton Plasma Physics Laboratory (US), Heliophysics (US)
National Science Foundation, U.S. Department of Energy, National Aeronautics and Space Administration, Nuclear Safety and Security Commission, Office of Science, Australian Research Council, Fusion Energy Sciences
Affordable and clean energy
Openalex Percentile: Top 34%
Ionosphere and magnetosphere dynamics
0.33
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O‐Mode Instability for Non‐Thermal Continuum Radiation Generated Near the Plasmapause — S. A. Boardsen, Iver H. Cairns, et al. · Journal of Geophysical Research Space Physics (2024) | TGRS Research Map | TGRS