Linear and nonlinear waves in dilute plasmas
- 1. Centre for Plasma-Astrophysics, K.U. Leuven, Celestijnenlaan 200B, B-3001 Heverlee (Belgium)
- 2. Space and Atmosphere Research Center, Department of Applied Mathematics, University of Sheffield, S3 7RH, Sheffield (United Kingdom)
Description
Small-amplitude magnetohydrodynamic (MHD) waves are studied in a dilute collisionless plasma with an anisotropic pressure distribution. The parallel and perpendicular pressure are defined with the aid of two polytropic pressure laws. For specific values of the polytropic indices, previous results obtained with the usual Chew-Goldberger-Low (CGL) double-adiabatic (i) and double-isothermal (ii) models are recovered. The double-polytropic model can be considered as the counterpart of the single-polytropic model. Dispersion relations for the linear waves are derived and analyzed in the presence of pressure anisotropy. The weakly nonlinear dynamics is shown to be governed by the Benjamin-Ono equation. The results are discussed in the CGL and double-isothermal limits
Additional details
Identifiers
- DOI
- 10.1063/1.1324935;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 537
- Journal Issue
- 1
- Journal Page Range
- p. 152-159
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- International conference on waves in dusty, solar, and space plasmas
- Dates
- 22-26 May 2000
- Place
- Leuven (Belgium)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 34072321
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Resource subtype / Literary indicator
- Conference, Numerical Data
- Descriptors DEI
- ALFVEN WAVES; MAGNETOHYDRODYNAMICS; PLASMA; PLASMA PRESSURE; PLASMA WAVES; SOLAR CORONA; SOUND WAVES; THEORETICAL DATA; WAVE PROPAGATION
- Descriptors DEC
- ATMOSPHERES; DATA; FLUID MECHANICS; HYDRODYNAMICS; HYDROMAGNETIC WAVES; INFORMATION; MECHANICS; NUMERICAL DATA; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE
Optional Information
- Notes
- (c) 2000 American Institute of Physics.