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Long-term variations in the geomagnetic activity level Part II: Ascending phases of sunspot cycles
Authors:V. Mussino  O. Borello Filisetti  M. Storini  H. Nevanlinna
Affiliation:1. Dipartimento di Fisica-Politecnico, Cso. Duca degli Abruzzi 24, I-10129, Torino, Italy
2. Raggi Cosmici-I.F.S.I.-CNR, c/o Dip. di Fisica-Univ. La Sapienza, P.le A. Moro 2, I-00185, Roma, Italy
3. Finnish Meteorological Institute, P.O. Box 503, SF-00101, Helsinki, Finland
Abstract:Monthly averages of the Helsinki Ak-values have been reduced to the equivalent aa-indices to extend the aa-data set back to 1844. A periodicity of about five cycles was found for the correlation coefficient (r) between geomagnetic indices and sunspot numbers for the ascending phases of sunspot cycles 9 to 22, confirming previous findings based on a minor number of sunspot cycles. The result is useful to researchers in topics related to solar-terrestrial physics, particularly for the interpretation of long-term trends in geomagnetic activity during the past, and to forecast geomagnetic activity levels in the future.
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