Published August 2007
| Version v1
Journal article
Generation of magnetoacoustic zonal flows by Alfven waves in a rotating plasma
Creators
- 1. Brazilian Center for Physics Research, Rua Xavier Sigaud, 150, 22290-180, Rio de Janeiro (Brazil)
- 2. Physics Institute, University of Sao Paulo, Cidade Universitaria, 05508-900, Sao Paulo (Brazil)
- 3. Institute of Nuclear Fusion, Russian Research Centre Kurchatov Institute, Kurchatov Square, 1, Moscow 123182 (Russian Federation)
- 4. University of Saskatchewan, 116 Science Place, Saskatoon S7N 5E2 (Canada)
- 5. Syzran Branch of Samara Technical University, 45, Sovetskaya Str., Syzran, Samara Region 446001 (Russian Federation)
- 6. Kharadze Abastumani National Astrophysical Observatory, 2a, Kazbegi Avenue, Tbilisi 0160 (Georgia)
- 7. Institute of Nuclear Fusion, Russian Research Centre Kurchatov Institute, 1, Kurchatov Square, Moscow 123182 (Russian Federation)
Description
Analytical theory of nonlinear generation of magnetoacoustic zonal flows in a rotating plasma is developed. As the primary modes causing such a generation, a totality of the Alfven waves are considered, along with the kinetic, inertial, and rotational. It is shown that in all these cases of the Alfven waves the generation is possible if the double plasma rotation frequency exceeds the zonal flow frequency
Additional details
Identifiers
- DOI
- 10.1063/1.2755941;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 14
- Journal Issue
- 8
- Journal Page Range
- p. 082302-082302.8
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 39086007
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALFVEN WAVES; MAGNETOHYDRODYNAMICS; NONLINEAR PROBLEMS; PLASMA INSTABILITY; PLASMA WAVES; ROTATING PLASMA; ROTATION
- Descriptors DEC
- FLUID MECHANICS; HYDRODYNAMICS; HYDROMAGNETIC WAVES; INSTABILITY; MECHANICS; MOTION; PLASMA
Optional Information
- Notes
- (c) 2007 American Institute of Physics