Published April 1977
| Version v1
Journal article
Solar magnetic fields and convection. IX
Description
The solar magnetic fields observed in active regions and their residues are thought to be parts of toroidal field systems renewed every 11-yr cycle from a poloidal field. The latter may be either a reversing (dynamo) field or a non-reversing, primordial field. The latter view was held for some 70 yr, but the apparent reversals of the polar-cap fields in 1957-8 and the development of dynamo theory brought wide acceptance of the former. Here evidence for and against each model is considered. (Auth.)
Additional details
Additional titles
- Subtitle (English)
- A primordial magnetic field
Identifiers
- DOI
- 10.1007/bf00642841;
Publishing Information
- Journal Title
- Astrophysics and Space Science
- Journal Volume
- 47
- Journal Issue
- 2
- Series
- Astrophys. Space Sci.
- Journal Page Range
- 319-340
- ISSN
- 0004-640X
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8331612
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CONVECTION; ECLIPSE; MAGNETIC FIELDS; MAGNETIC FLUX; SOLAR CORONA; SOLAR CYCLE; STAR MODELS; SUN; ZEEMAN EFFECT
- Descriptors DEC
- ENERGY TRANSFER; HEAT TRANSFER; MATHEMATICAL MODELS; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent