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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 16, issue 7
Ann. Geophys., 16, 804–811, 1998
© European Geosciences Union 1998
Ann. Geophys., 16, 804–811, 1998
© European Geosciences Union 1998

  31 Jul 1998

31 Jul 1998

Spectrum of geomagnetic activity in the period range 5−60 days: possible lunar influences

J. Střeštík J. Střeštík
  • Geophysical Institute, Acad. Sci. of the Czech Rep., Boční II 1401, Praha 4 - Spořilov, CZ-14131, Czech Republic
  • Fax: + 42 2 71 76 15 49; e-mail: jstr@ig. cas. cz

Abstract. The series of daily Ap-indices has been subdivided into pentades (1932–1936 etc.) and spectra with fine-frequency resolution have been calculated for the indices in each of these intervals. Daily sunspot numbers have been processed in the same way. The average spectrum from all spectra in the pentades, as well as the spectrum from the whole interval have been calculated, and significant peaks have been determined. There is a significant difference between the spectra in the pentades containing the solar activity minimum (1932–1936, 1942–1946 etc.) and those containing the solar activity maximum (1937–1941, 1947–1951 etc.). Most peaks can be interpreted as a response to solar rotation and to the structure of solar wind speed (two high-speed streams per solar rotation), both modulated by the 11-year, annual and semi-annual waves. No significant peak corresponding to the period of the synodic month, or its half has been found. This result suggests that the influence of lunar cycles on some natural phenomena (if any) is not mediated by geomagnetic activity.

Key words. Geomagnetism and paleomagnetism · Time variations · Diurnal to secular · Magnetospheric physics · Solar wind-magnetosphere interactions

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