Published April 1982
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Dynamo theory: can amplification of magnetic-field profiles arise from a cross-field alpha effect
Description
The answer to the title question is here provided in cylindrical geometry for an essentially arbitrary radial dependence of this alpha effect, except that it is subject to a simple, physically required constraint. The interest in this type of alpha effect derives from its connection with compressible turbulence, which is usually not considered in kinematic dynamo theory
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS., PC A02/MF A01 as DE82013739.Files
14718398.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 8 p.
- Report number
- LA--9290-MS
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 14718398
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- MAGNETIC FIELD CONFIGURATIONS; MAGNETIC FIELD REVERSAL; PLASMA; REVERSE-FIELD PINCH; SYMMETRY; TIME DEPENDENCE
- Descriptors DEC
- PINCH EFFECT