Plasma heating by spatial resonance of Alfven wave
Description
Heating of a collisionless plasma by utilizing the spatial resonance of shear Alfvén waves is proposed and application to toroidal plasmas is discussed. The resonance exists due to the nonuniform Alfvén speed. This heating scheme is analyzed in one dimension including the effects of a shear magnetic field and plasma compressibility. For plasmas with smooth nonuniformities (| k⊥l | ≫ 1, k⊥ is the wavenumber prependicular to the ambient magnetic field and the nonuniformity direction, and l is the scale length of the nonuniformity), the energy absorbed per unit surface area per driving cycle is [b02(μ0k⊥)−1]. Here, b0 is the flux density of the driving magnetic field evaluated at the resonant point. With sharp nonuniformities (| k⊥l | ≪ 1), absorption is large if the surface eigenmode is excited. The corresponding value is [b02(μ0k⊥)−1(k⊥l)−1]. Otherwise, it is [b02(μ0k⊥)−1(k⊥l)].
Additional details
Identifiers
- DOI
- 10.1063/1.1694904;
Publishing Information
- Journal Title
- The Physics of Fluids
- Journal Volume
- 17
- Journal Issue
- 7
- Series
- Phys. Fluids.
- Journal Page Range
- 1399-1403
- ISSN
- 0031-9171
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 6166910
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ALFVEN WAVES; ANALYTICAL SOLUTION; BOUNDARY CONDITIONS; COLLISIONLESS PLASMA; PLASMA HEATING; RESONANCE ABSORPTION; TOROIDAL CONFIGURATION
- Descriptors DEC
- ABSORPTION; ANNULAR SPACE; CONFIGURATION; HEATING; HYDROMAGNETIC WAVES; PLASMA
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent