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The behaviour of prominence areas in the 11-Year cycle and their relationship with other solar events

✍ Scribed by M. N. Gnevyshev; V. I. Makarov


Publisher
Springer
Year
1985
Tongue
English
Weight
206 KB
Volume
95
Category
Article
ISSN
0038-0938

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✦ Synopsis


On the basis of the data on prominence areas for 1880-1976 and positions of the boundary background magnetic field for 1955-1982 it is shown that the maximum development of prominences and their poleward migration, accompanied by the magnetic field reversal, concides with the first maximum of the 11-year solar cycle, which is characterized by an enhancement of solar activity at ~ll latitudes. The second maximum is an increase of all features, including prominences but in the low latitudes only. That prominence zone migrates poleward in the following 11-year solar cycle.