Solar Physics

, Volume 248, Issue 1, pp 203–209

Prediction of Solar Cycle Maximum Using Solar Cycle Lengths

Authors

    • Instituto Nacional de Pesquisas Espacias
Article

DOI: 10.1007/s11207-008-9125-8

Cite this article as:
Kane, R.P. Sol Phys (2008) 248: 203. doi:10.1007/s11207-008-9125-8

Abstract

If the rise time RT, fall time FT, and total time TT (i.e., RT+FT) of a solar cycle are compared against the maximum amplitude Rz(max ) for the following cycle, then only the association between TT and Rz(max ) is inferred to be well anticorrelated, inferring that the larger (smaller) the value of Rz(max ) for the following cycle, the shorter (longer) the TT of the preceding cycle. Although the inferred correlation (−0.68) is statistically significant, the inferred standard error of estimate is quite large, so predictions using the inferred correlation are not very precise. Removal of cycle pairs 15/16, 19/20, and 20/21 (statistical outliers) yields a regression that is highly statistically significant (−0.85) and reduces the standard error of estimate by 18%. On the basis of the adjusted regression and presuming TT=140 months for cycle 23, the present ongoing cycle, cycle 24’s 90% prediction interval for Rz(max ) is estimated to be about 94±44, inferring only a 5% probability that its Rz(max ) will be larger than about 140, unless of course cycle pair 23/24 is a statistical outlier.

Copyright information

© Springer Science+Business Media B.V. 2008