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A new method of very long-term prediction of solar activityA method of solar activity prediction based on the statistical relationship between the minimum value of geomagnetic activity in each 11 year cycle and the height of the next sunspot cycle is proposed. The method is applied to predict sunspot cycle 21.
Document ID
19800016204
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ohl, A. I. (Main Astronomical Observatory Pulkovo, Ussr)
Ohl, G. I. (Arkticheskii i Antarkticheskii Nauchno-Issled. Inst.)
Date Acquired
August 10, 2013
Publication Date
December 1, 1979
Publication Information
Publication: NASA. Marshall Space Flight Center Solar-Terrest. Predictions Proc., Vol. 2
Subject Category
Solar Physics
Accession Number
80N24697
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19800016185Collected WorksSolar-terrestrial Predictions Proceedings. Volume 2: Working Group Reports and Reviews
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