Topology of the magnetic field and geomagnetism.
Abstract
We define the topology of an (axisymmetric) magnetic field, a set of qualitative labels characterizing the connectivity of the lines of force. Under the special continuous deformations of theB-field defined by time evolution under the dynamo equation in the 'convective' regime (where the frozen-in behavior dominates the diffusion), this topology is preserved. This theorem should have applications to the study of time-varying magnetic fields in that regime in the case that exact or even approximate solutions are difficult to obtain. A partial generalization to the general case of convection and diffusion is made. As an application, a critique of Hibberd's recent theory of a time-dependent axisymmetric geomagnetic dynamo whose dipole-like field undergoes successive reversals is given.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- July 1981
- DOI:
- 10.1007/BF00649471
- Bibcode:
- 1981Ap&SS..77..455I
- Keywords:
-
- Dynamo Theory;
- Geomagnetism;
- Magnetic Field Configurations;
- Topology;
- Earth Surface;
- Interstellar Magnetic Fields;
- Lines Of Force;
- Neutral Currents;
- Telluric Currents;
- Geophysics;
- Magnetic Field;
- Convection;
- Time Evolution;
- Approximate Solution;
- Recent Theory;
- Dynamo Theory:Geomagnetic Field