The spectrum of the Parker equations
Abstract
The distribution and evolution of the large-scale solar magnetic field is considered in the framework of a Parker dynamo model. The complete discrete spectrum of the dynamo waves is found. The spectral solution is found for the case of large dynamo numbers using the WKB (quasi-classical) approximation.
- Publication:
-
Astronomy Reports
- Pub Date:
- January 1998
- Bibcode:
- 1998ARep...42..127G