DocumentCode
2570862
Title
Quasineutral Particle/Fluid Hybrid Simulation Technique for Whistlers
Author
Lampe, M. ; Ganguli, G. ; Joyce, G. ; Manheimer, W. ; Streltsov, A.
Author_Institution
Div. of Plasma Phys., Naval Res. Lab., Washington, DC
fYear
2005
fDate
20-23 June 2005
Firstpage
246
Lastpage
246
Abstract
Summary form only given. We have developed a new simulation scheme for whistlers and other slow EM waves which is fully kinetic and fully nonlinear, works in homogeneous or inhomogeneous situations, is not restricted to a single coherent mode, eliminates the speed-of-light time scale and the electron plasma oscillation time scale, and concentrates simulation resources on the parts of the electron distribution that make kinetic contributions to wave growth. The elements of the scheme are as follows. (1) The plasma is represented as a cold fluid plus a set of simulation particles. The simulation particles can be chosen to represent any part of the electron velocity distribution that is of kinetic interest, e.g. the complete ensemble of energetic electrons, or only a set of resonant electrons. (2) Quasineutrality (QN) is assumed, i.e. div J=0. We emphasize that this does not mean that there are no electrostatic fields, only that the electric field E is determined by QN, rather than by Poisson´s equation. This assumption is appropriate when the frequencies are slow compared to the plasma frequency, and it eliminates plasma oscillations. (3) The displacement current is neglected, since the waves of interest are slow compared to c. This is similar to the Darwin model. However, (1) and (2) allow us to neglect the fall displacement current, not just the solenoidal part, and thereby avoid all of the complications of the Darwin model. (4) Faraday´s and Ampere´s laws, rather than a momentum conservation equation, are used to push the cold fluid velocity. This guarantees QN. (5) The simulation particles are pushed in standard PIC fashion. (6) The magnetic field is determined by Ampere´s law. In the linear regime, the scheme reproduces the quasi-longitudinal dispersion relation for whistlers, and is accurate for propagation angles up to the resonance cone. An extremely stable and accurate predictor-corrector scheme is used, and energy is conserved to great accuracy. The cod- need not resolve spatial scales smaller than the wavelengths of interest, nor time scales shorter than the gyrofrequency. We have used the code to study long-time nonlinear evolution of whistler instabilities; results will be shown for a variety of situations
Keywords
dispersion relations; plasma electromagnetic wave propagation; plasma instability; plasma nonlinear waves; plasma simulation; predictor-corrector methods; whistlers; Ampere law; Faraday law; Poisson equation; cold fluid velocity; displacement current; electron plasma oscillation time scale; electron velocity distribution; electrostatic fields; momentum conservation equation; plasma frequency; predictor-corrector scheme; quasilongitudinal dispersion relation; quasineutral particle-fluid hybrid simulation; speed-of-light time scale; whistler instabilities; Dispersion; Electrons; Electrostatics; Frequency; Kinetic theory; Magnetic fields; Plasma simulation; Plasma waves; Poisson equations; Resonance;
fLanguage
English
Publisher
ieee
Conference_Titel
Plasma Science, 2005. ICOPS '05. IEEE Conference Record - Abstracts. IEEE International Conference on
Conference_Location
Monterey, CA
ISSN
0730-9244
Print_ISBN
0-7803-9300-7
Type
conf
DOI
10.1109/PLASMA.2005.359319
Filename
4198578
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