Published 1987
| Version v1
Journal article
On the oscillatory behaviour of kinematic mean-field dynamos
Creators
- 1. Akademie der Wissenschaften der DDR, Potsdam. Zentralinstitut fuer Astrophysik
- 2. Akademie der Wissenschaften der DDR, Sonneberg. Zentralinstitut fuer Astrophysik
Description
The paper considers the question after the circumstances in which kinematic mean-field dynamos can have oscillatory magnetic field modes. The conducting fluid body is allowed to be of almost arbitrary shape; its surroundings are vacuum. A general relation for the frequency of oscillation is derived. This relation is discussed more closely for models with pure α2-mechanism. Proof is given that no oscillations can occur for constant α. The investigations published so far on spherical models with pure α2-mechanism call up the question whether there is a chance for axisymmetric modes to be oscillatory. For both spherical models and disk models the possibility of oscillatory axisymmetric modes is demonstrated by examples. (author)
Additional details
Publishing Information
- Journal Title
- Astron. Nachr.
- Journal Volume
- 308
- Journal Issue
- 2
- Series
- Astron. Nachr.
- Journal Page Range
- 101-109
- ISSN
- 0004-6337
- CODEN
- ASNAA
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- German Democratic Republic
- INIS RN
- 18084258
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANALYTICAL SOLUTION; ANISOTROPY; AXIAL SYMMETRY; BOUNDARY CONDITIONS; COSMOLOGICAL MODELS; CYLINDERS; EIGENVALUES; FLUIDS; MAGNETIC FIELDS; MEAN-FIELD THEORY; OSCILLATIONS; SPHERES; STEADY-STATE CONDITIONS; TRAVELLING WAVES
- Descriptors DEC
- MATHEMATICAL MODELS; SYMMETRY