The Interplay of the Solar Wind Core and Suprathermal Electrons: A Quasilinear Approach for Firehose Instability
arXiv:1901.11406 · doi:10.3847/1538-4357/aaf72d
Abstract
In the solar wind an equipartition of kinetic energy densities can be easily established between thermal and suprathermal electrons and the instability conditions are markedly altered by the interplay of these two populations. The new thresholds derived here for the periodic branch of firehose instability shape the limits of temperature anisotropy reported by the observations for both electron populations. This instability constraint is particularly important for the suprathermal electrons which, by comparison to thermal populations, are even less controlled by the particle-particle collisions. An extended quasilinear approach of this instability confirms predictions from linear theory and unveil the mutual effects of thermal and suprathermal electrons in the relaxation of their temperature anisotropies and the saturation of growing fluctuations.
ApJ in press
References in corpus (3)
Cited by in corpus (11)
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- Electron Temperature Anisotropy and Electron Beam Constraints From Electron Kinetic Instabilities in the Solar Wind
- Whistler instabilities from the interplay of electron anisotropies in space plasmas: A quasilinear approach
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- Decoding the formation of hammerhead ion populations observed by Parker Solar Probe
- Numerical simulations of temperature anisotropy instabilities stimulated by suprathermal protons
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