Published April 1976 | Version v1
Journal article

22-year cycle or 11-year cycle in the latitude drift of sunspot groups

Creators

  • 1. Helsinki Univ. (Finland). Observatory and Astrophysics Lab.

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

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
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