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Marginal stability of whistler-mode waves in plasma with multiple electron populations

Physics of Plasmas. 2022. Vol. 29. No. 5. Article 052901.
V. A. Frantsuzov, Artemyev A. V., P. I. Shustov, Zhang X.

Whistler-mode waves are one of the most intense electromagnetic waves in the planetary magnetospheres. These waves are responsible for energetic electron losses into the atmosphere and for electron acceleration up to relativistic energies. Generation of whistler-mode waves is typically attributed to the thermal electron anisotropy. The anisotropy corresponding to the marginal stability for whistler-mode waves has been derived for a single-component Maxwellian plasma, but this criterion does not always work in the Earth’s magnetosphere where whistler-mode waves are generated by an energy-confined, strongly anisotropic electron population. This study aims to generalize the marginal stability equation for multi-component plasma with a small, but strongly anisotropic, electron population. New analytical equations for the marginal stability have been derived from the linear analysis. We have also discussed applicability of the derived equations for different electron populations in the Earth’s magnetosphere.

Research target: Physics
Language: English
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Keywords: linear theoryлинейная теорияspace plasma physics2772 plasma waves and instabilitiesФизика плазмысвистовые волныплазменные волны и неустойчивостьWhistler wavesисследования космоса
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