Published June 2008
| Version v1
Journal article
Parametric instabilities of Alfven waves in a multispecies plasma: Kinetic effects
Creators
- 1. Departamento de Fisica, Facultad de Ciencias Fisicas y Matematicas, Universidad de Concepcion, Casilla 160-C, Concepcion (Chile)
Description
Parametric instabilities of a circularly polarized Alfven wave in a multispecies magnetized plasma are considered. An analytic kinetic description and hybrid simulations for the linear behavior of the instabilities are given. It is found that, even for low-β regimes, both the kinetic effects and the presence of heavy ions substantially modify the characteristics of parametric instabilities as compared to the fluid model. The decay instability can be severely quenched in a plasma composed of massless electrons, protons, and alpha particles when the alphas are slightly hotter than the protons. These results could be important in describing the heating processes of heavy ions in the solar corona
Additional details
Identifiers
- DOI
- 10.1063/1.2932113;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 15
- Journal Issue
- 6
- Journal Page Range
- p. 062106-062106.8
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40002940
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALFVEN WAVES; ALPHA PARTICLES; DECAY INSTABILITY; ELECTRONS; HEAVY IONS; PARAMETRIC INSTABILITIES; PLASMA; PLASMA HEATING; PROTONS; SIMULATION; SOLAR CORONA
- Descriptors DEC
- ATMOSPHERES; BARYONS; CHARGED PARTICLES; ELEMENTARY PARTICLES; FERMIONS; HADRONS; HEATING; HYDROMAGNETIC WAVES; INSTABILITY; IONIZING RADIATIONS; IONS; LEPTONS; NUCLEONS; PLASMA INSTABILITY; PLASMA MACROINSTABILITIES; RADIATIONS; SOLAR ATMOSPHERE; STELLAR ATMOSPHERES; STELLAR CORONAE
Optional Information
- Notes
- (c) 2008 American Institute of Physics