Computer Science
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001kfnt...17..348l&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, vol. 17, no. 4, p. 348-356
Computer Science
Scientific paper
We analyze the power spectra of both the solar mean magnetic field (SMMF) time series (magnetograph measurements at Stanford, cycles 21 and 22) as well as the N(+) and S(-) components in the entire frequency range. Separate investigation of the N(+) and S(-) component spectra shows a detailed pattern of space-time organization of large-scale magnetic fields on the time scale of one cycle and within cycles. Significant differences between the cycle power spectra point to variations in the magnetic structure space-time organization with cycle. The difference between the N(+) and S(-) component spectra within cycles defines the magnetic asymmetry.
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