Published October 1984
| Version v1
Journal article
Sunspot pair formation by the photospheric dynamo process
Description
It is suggested that the formation of a pair of sunspots results from amplification of the weak, large-scale fields in the photosphere, rather than from emergence of a hypothetical magnetic flux ''tube'' from beneath the photosphere. (author)
Additional details
Publishing Information
- Journal Title
- Planet. Space Sci.
- Journal Volume
- 32
- Journal Issue
- 10
- Series
- Planet. Space Sci.
- Journal Page Range
- 1257-1261
- ISSN
- 0032-0633
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 16019303
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DYNAMICS; MAGNETIC FIELDS; PHOTOSPHERE; SOLAR FLARES; SUNSPOTS
- Descriptors DEC
- ATMOSPHERES; MECHANICS; SOLAR ACTIVITY; SOLAR ATMOSPHERE; STARSPOTS; STELLAR ACTIVITY; STELLAR ATMOSPHERES; STELLAR FLARES