Counterstreaming magnetized plasmas. I. Parallel wave propagation
Creators
- 1. Institut fuer Theoretische Physik, Lehrstuhl IV: Weltraum- und Astrophysik, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
Description
The properties of longitudinal and transverse oscillations in magnetized counterstreaming Maxwellian plasmas of arbitrary composition and different thermal velocities for waves propagating parallel to the stream direction are investigated on the basis of the Maxwell equations and the relativistic Vlasov equation. These dispersion relations describe the linear response of the system to the initial perturbations and thus define all existing linear parallel propagating plasma modes in the system. The dispersion relations hold for nonrelativistic values of the plasma temperatures, streaming velocities, and for any values of the relative intensities of the two streams and for all wave-number and frequency values of the oscillations. All dispersion relations are expressed in terms of the well-documented Fried and Conte plasma dispersion function and are thus valid for the whole complex-frequency plane, which assures the validity of growth and damping rates
Additional details
Identifiers
- DOI
- 10.1063/1.2139505;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 12
- Journal Issue
- 12
- Journal Page Range
- p. 122901-122901.7
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37085616
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- BOLTZMANN-VLASOV EQUATION; CHARGED-PARTICLE TRANSPORT; DAMPING; DISPERSION RELATIONS; DISTURBANCES; ELECTRON TEMPERATURE; ION TEMPERATURE; MAXWELL EQUATIONS; OSCILLATIONS; PLASMA INSTABILITY; PLASMA WAVES; RELATIVISTIC PLASMA; RELATIVISTIC RANGE; VELOCITY; WAVE PROPAGATION
- Descriptors DEC
- DIFFERENTIAL EQUATIONS; ENERGY RANGE; EQUATIONS; INSTABILITY; PARTIAL DIFFERENTIAL EQUATIONS; PLASMA; RADIATION TRANSPORT
Optional Information
- Notes
- (c) 2005 American Institute of Physics