A wavelet analysis of solar mean magnetic field measurements

Details A wavelet analysis of solar mean magnetic field measurements A wavelet analysis of solar mean magnetic field measurements

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.477...79b&link_type=abstract

In: Proceedings of the Second Solar Cycle and Space Weather Euroconference, 24 - 29 September 2001, Vico Equense, Italy. Editor:

Physics

2

Solar Activity, Solar Mean Magnetic Field, Wavelets

Scientific paper

Solar mean magnetic field (SMMF) measurements from the Wilcox Solar Observatory and with SOHO/MDI are analyzed using continuous wavelet transforms, SMMF variability is found at a number of temporal scales. Detected SMMF variations with a 1-2 year period is considered to be linked to long-term variations in the internal rotation of the Sun. Intermediate SMMF oscillations with a period of 80-200 days are probably connected to the evolution of large active regions. We also find evidence for 90 minute variations with coronal mass ejections as a probable origin.

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