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The migration of sunspot activity along solar meridians and parallels
Published online by Cambridge University Press: 14 August 2015
Abstract
The places of local maxima of sunspot activity, i.e. the formation of solar active regions, seem to follow in a definite sequence of tracks over the Sun's surface. These sequences of activity apparently represent distinct continuous streams, whose duration may be of the order of magnitude of 1 year.
- Type
- Part I: General Development of an Active Region
- Information
- Copyright
- Copyright © Reidel 1968