22-year cycle or 11-year cycle in the latitude drift of sunspot groups
Description
Some earlier investigations seem to indicate that sunspots show an average drift in latitude which varies sinusoidially with the period of the double sunspot cycle (about 22 years), while the same investigations do not show similar variability with the period of the single sunspot cycle (about 11 years). Other studies, however, show that the drift of sunspots varies with the period of the single sunspot cycle. There seems to be a discrepancy between the two results. The problem is reinvestigated on the basis of long-lived sunspot groups, but treating the material in a way different from that used before. This procedure, which uses central values of the proper motions of the groups instead of their average values, gives an additional proof of the reality of the 11-year period of the drift. It also seems to produce the 22-year period, but there is such a difference between the variabilities of the drift found on the basis of the two methods that the 22-year cycle of the drift is made doubtful. (Auth.)
Additional details
Identifiers
- DOI
- 10.1007/bf00154762;
Publishing Information
- Journal Title
- Solar Physics
- Journal Volume
- 47
- Journal Issue
- 2
- Series
- Sol. Phys.
- Journal Page Range
- 541-550
- ISSN
- 0038-0938
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- Netherlands
- INIS RN
- 8308748
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data
- Descriptors DEI
- DATA; MOTION; SOLAR CYCLE; SUN; SUNSPOTS
- Descriptors DEC
- INFORMATION; SOLAR ACTIVITY; STARS
Optional Information
- Notes
- Updated automatically by Metadata and Full-Text Enrichment Agent