The strong Langmuir turbulence spectra in weakly relativistic plasma
Source abstract
Abstract
The spectral characteristics of strong Langmuir turbulence in weakly relativistic plasma is analyzed. The temporal evolutions of the turbulence energy density spectra are obtained by perfoyming the fast Fourier transformations on weakly relativistic Zakharov equations. The relativity parameter significantly influenced the Langmuir turbulence, in that a decrease in the relativity parameter lengthened the action time of wave-wave and wave-particle interactions, which is useful for studying the particles acceleration problem.
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Research context
OpenAlex topics: Ionosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Magnetic confinement fusion research
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Department of Physics, Nanchang University 1 , Jiangxi, Nanchang 330031, China
College of Nuclear Science and Technology, Beijing Normal University 2 , Beijing 100875, China
Funding
jiangxi province key laboratory of fusion and information control · Natural Science Foundation of Jiangxi Province · National Natural Science Foundation of China
References (22)
Show source-provided references
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