Simulation of collisionless electrostatic velocity-shear-driven instabilities
Creators
- 1. Department of Physics and Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California 90024-1547 (United States)
Description
The properties of electrostatic instabilities in velocity shear layers in collisionless plasmas are investigated by means of two-dimensional particle simulations for the case where the ion gyroradius is comparable to the scale length of the velocity shear. For modes exactly perpendicular to the magnetic field, the Kelvin--Helmholtz instability dominates the evolution of the system producing eφ/Te>1; the observed growth rates show no reduction compared to the hydromagnetic limit. To obtain this result for the case of negative shear (v0y'/Ωi<0), it is necessary to include the kinetic modifications to the structure of the shear layer equilibrium. For finite kparallel in the range 0<kparallel/k<0.04, the shorter-wavelength inhomogeneous-energy-density-driven instability cannot be identified in the simulations, and the upper limit on its excitation is eφ/Te approx-lt 2x10-3
Additional details
Publishing Information
- Journal Title
- Physics of Fluids B
- Journal Volume
- 5
- Journal Issue
- 10
- Journal Page Range
- p. 3770-3778.
- ISSN
- 0899-8221
- CODEN
- PFBPEI
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 25013275
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- COLLISIONLESS PLASMA; ELECTROSTATICS; HELMHOLTZ INSTABILITY; INSTABILITY GROWTH RATES; MAGNETOPAUSE; PLASMA MACROINSTABILITIES; PLASMA SIMULATION; SHEAR; SOLAR WIND
- Descriptors DEC
- INSTABILITY; PLASMA; PLASMA INSTABILITY; SIMULATION; SOLAR ACTIVITY; STELLAR ACTIVITY; STELLAR WINDS