Published October 20, 2000 | Version v1
Journal article

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

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.