Published January 2005
| Version v1
Journal article
Excitation of zonal flows by kinetic Alfven waves
Creators
- 1. Innovative Science Applications and Technology, Via S. Pellico 19, Saluzzo (Italy)
- 2. Department of Electrical and Computer Engineering, University of California, San Diego, La Jolla, California 92003 (United States)
- 3. Department of Physics, Umeaa University, SE-90187 Umeaa (Sweden)
- 4. Institut fuer Theoretische Physik IV and Centre for Plasma Science and Astrophysics, Fakultaet fuer Physik und Astronomie, Ruhr-Universitaet Bochum, D-44780 Bochum (Germany)
Description
Nonlinear couplings between dispersive kinetic Alfven waves (DKAWs) and electrostatic convective cells/zonal flows are reexamined. A set of equations that exhibit nonlinear couplings between the scalar and parallel vector potentials of the DKAWs and the scalar potential of zonal flows that are reinforced by the Reynolds stresses of the DKAWs in a magnetized plasma is presented. The equations are then Fourier-analyzed to obtain the nonlinear dispersion relation. The latter exhibits modulational instabilities, which could be responsible for enhanced zonal flows in a uniform magnetized plasma. Zonal flows can regulate the transport of plasma particles in laboratory magnetoplasmas as well as in the Earth's magnetosphere and in the solar corona
Additional details
Identifiers
- DOI
- 10.1063/1.1826095;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 12
- Journal Issue
- 1
- Journal Page Range
- p. 012310-012310.4
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 36096731
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALFVEN WAVES; DISPERSION RELATIONS; EARTH MAGNETOSPHERE; FOURIER ANALYSIS; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; PLASMA; PLASMA INSTABILITY; SOLAR CORONA
- Descriptors DEC
- ATMOSPHERES; EARTH ATMOSPHERE; FLUID MECHANICS; HYDRODYNAMICS; HYDROMAGNETIC WAVES; INSTABILITY; MECHANICS; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE
Optional Information
- Notes
- (c) 2005 American Institute of Physics