The probable behaviour of sunspot Cycle 21
โ Scribed by W. Gleissberg
- Publisher
- Springer
- Year
- 1971
- Tongue
- English
- Weight
- 292 KB
- Volume
- 21
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
Regarding new bipolar magnetic regions as sources of flux, we have simulated the evolution of the radial component of the solar photospheric magnetic field during 1976-1984 and derived the corresponding evolution of the line-of-sight polar fields as seen from Earth. The observed timing and strength
The sunspot record for the time interval 1749-1977 can be represented conveniently by an harmonic model comprising a relatively large number of lines. Solar activity can otherwise be considered as a sequence of partly overlapping events, triggered periodically at intervals of the order of 11 years.