Spectral analysis of sunspot number and geomagnetic indices (1868 2001)

Details Spectral analysis of sunspot number and geomagnetic indices (1868 2001) Spectral analysis of sunspot number and geomagnetic indices (1868 2001)

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jastp..68..182p&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 68, Issue 2, p. 182-190.

Physics

11

Scientific paper

The multiple-taper spectral analysis was applied to aa, Ap and Rz annual and monthly average series (1868 2001). The significant periods at 95% confidence level for annual averages are 11.1 and 10.2 years for Rz and 11.1, 5.3, 4.3, 2.7 and 2.1 years for aa. For monthly averages, the significant periods were 133 (11.1 years) and 17.7 months for Rz and 133 (11.1 years), 63.7 (5.3 years), 17.5, 12.7 and 6 months for aa. The periods associated with the solar cycle are observed in both series. The aa spectrum showed in addition a peak near 4.3 years, which is not present in the Rz spectrum. Other works have also shown this peak in geomagnetic activity. This peak is believed to be caused by the dual-peak structure in the aa. The 22-year Hale cycle was not detected either in Rz or aa spectrum in the period 1868 2001, but it was seen in Rz data for 1700 2000 annual averages. The explanation of this 22-year cycle has been questioned and while in some spectral analysis this periodicity has been found, others have failed in its detection. The aa spectrum showed in addition a peak of 6 months, associated to the semi-annual variation of geomagnetic activity. Three hypotheses have been considered to explain the seasonal activity variation. These are the Russell McPherron effect, the equinoctial effect and the axial effect.

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