Published April 1977 | Version v1
Journal article

Solar magnetic fields and convection. IX

  • 1. National Measurement Lab., Sydney (Australia)

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.)

Part of:
Solar magnetic fields and convection. VIII

Additional details

Additional titles

Subtitle (English)
A primordial magnetic field

Identifiers

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
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