Marshall Technical Reports Server

An Examination of Selected Geomagnetic Indices in Relation
to the Sunspot Cycle

NASA/TP-2006–214711, Wilson, Robert M. and Hathaway, David H., An Examination of Selected Geomagnetic Indices in Relation
to the Sunspot Cycle
, George C. Marshall Space Flight Center Marshall Space Flight Center, AL 35812, National Aeronautics and Space Administration Washington, DC 20546–0001, December 2006, pp. 52, Format(s): PDF 1880k


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Previous studies have shown geomagnetic indices to be useful for providing early estimates for the size of the following sunspot cycle several years in advance. Examined in this study are various precursor methods for predicting the minimum and maximum amplitude of the following sunspot cycle, these precursors based on the aa and Ap geomagnetic indices and the number of disturbed days (NDD), days when the daily Ap index equaled or exceeded 25. Also examined is the yearly peak of the daily Ap index (Apmax), the number of days when Ap ≥ 100, cyclic averages of sunspot number R, aa, Ap, NDD, and the number of sudden storm commencements (NSSC), as well the cyclic sums of NDD and NSSC. The analysis yields 90-percent prediction intervals for both the minimum and maximum amplitudes for cycle 24, the next sunspot cycle. In terms of yearly averages, the best regressions give Rmin = 9.8 ± 2.9 and Rmax = 153.8 ± 24.7, equivalent to Rm = 8.8 ± 2.8 and RM = 159 ± 25.5, based on the 12-mo moving average (or smoothed monthly mean sunspot number). Hence, cycle 24 is expected to be above average in size, similar to cycles 21 and 22, producing more than 300 sudden storm commencements and more than 560 disturbed days, of which about 25 will be Ap ≥100. On the basis of annual averages, the sunspot minimum year for cycle 24 will be either 2006 or 2007.
Keywords:sun, sunspot cycle, solar cycle prediction, geomagnetic indices
Subjects:Space Sciences: Solar Physics
ID Code:741
Deposited On:22 May 2007