Computer Science
Scientific paper
Feb 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sosyr..42...63s&link_type=abstract
Solar System Research, Volume 42, Issue 1, pp.63-71
Computer Science
1
96.60.Qd, Sun Spots, Solar Cycles
Scientific paper
The reconstructed part of the series of monthly mean Wolf numbers (for the period from 1749 to 1849) is estimated, and a conclusion about its irregular character is made. The estimation criteria are taken from the properties of the remaining part of the Wolf series (1849-2004). The further analysis of the components of the latter series made it possible to choose a transformation leading to the regularization of the solar-cycle characteristics and, as a consequence, to their model description. The cycle properties are differentiated by their parity and the broken relation of the maxima of cycles 22 and 23 is restored. The long-period component of the series (from 1849 to 2004) is interpolated by a sinusoidal function with a period of ˜150 years. This allows us to perform an inverse transformation on an external time interval and correct the reconstructed part of the Wolf series.
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