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A physical mechanism for the prediction of the sunspot number during solar cycle 21On physical grounds it is suggested that the sun's polar field strength near a solar minimum is closely related to the following cycle's solar activity. Four methods of estimating the sun's polar magnetic field strength near solar minimum are employed to provide an estimate of cycle 21's yearly mean sunspot number at solar maximum of 140 plus or minus 20. This estimate is considered to be a first order attempt to predict the cycle's activity using one parameter of physical importance.
Document ID
19780021085
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Schatten, K. H.
(Stanford Univ. CA, United States)
Scherrer, P. H.
(Stanford Univ. CA, United States)
Svalgaard, L.
(Stanford Univ. CA, United States)
Wilcox, J. M.
(Stanford Univ. CA, United States)
Date Acquired
September 3, 2013
Publication Date
February 1, 1978
Subject Category
Solar Physics
Report/Patent Number
SU-IPR-736
NASA-CR-157320
Report Number: SU-IPR-736
Report Number: NASA-CR-157320
Accession Number
78N29028
Funding Number(s)
CONTRACT_GRANT: N00014-76-C-0207
CONTRACT_GRANT: NSF ATM-77-20580
CONTRACT_GRANT: NGR-05-020-559
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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