Electron phase-space hole transverse instability at high magnetic field

Analytic treatment is presented of the electrostatic instability of an initially planar electron hole in a plasma of effectively infinite particle magnetization. It is shown that there is an unstable mode consisting of a rigid shift of the hole in the trapping direction. Its low frequency is determi...

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Bibliographic Details
Main Author: Hutchinson, Ian H. (Author)
Other Authors: Massachusetts Institute of Technology. Department of Mathematics (Contributor)
Format: Article
Language:English
Published: Cambridge University Press (CUP), 2020-03-25T17:37:10Z.
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Online Access:Get fulltext
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100 1 0 |a Hutchinson, Ian H.  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Mathematics  |e contributor 
245 0 0 |a Electron phase-space hole transverse instability at high magnetic field 
260 |b Cambridge University Press (CUP),   |c 2020-03-25T17:37:10Z. 
856 |z Get fulltext  |u https://hdl.handle.net/1721.1/124325 
520 |a Analytic treatment is presented of the electrostatic instability of an initially planar electron hole in a plasma of effectively infinite particle magnetization. It is shown that there is an unstable mode consisting of a rigid shift of the hole in the trapping direction. Its low frequency is determined by the real part of the force balance between the Maxwell stress arising from the transverse wavenumber and the kinematic jetting from the hole's acceleration. The very low growth rate arises from a delicate balance in the imaginary part of the force between the passing-particle jetting, which is destabilizing, and the resonant response of the trapped particles, which is stabilizing. Nearly universal scalings of the complex frequency and with hole depth are derived. Particle in cell simulations show that the slow-growing instabilities previously investigated as coupled hole-wave phenomena occur at the predicted frequency, but with growth rates 2 to 4 times greater than the analytic prediction. This higher rate may be caused by a reduced resonant stabilization because of numerical phase-space diffusion in the simulations. ©2019 Keywords: plasma instabilities; plasma nonlinear phenomena; space plasma physics 
520 |a NASA (Grant NNX16AG82G) 
546 |a en 
655 7 |a Article 
773 |t 10.1017/S0022377819000564 
773 |t Journal of Plasma Physics