@Article{Kane:1999:PrSuMa,
author = "Kane, Rajaram Purushottam",
title = "Prediction of the sunspot maximum of solar cycle 23 by
extrapolation of spectral components",
journal = "Solar Physics",
year = "1999",
volume = "189",
number = "1",
pages = "217--224",
keywords = "GEOF{\'{\I}}SICA ESPACIAL, ciclos solar, manchas solares,
m{\'e}todo de entropia m{\'a}xima, solar cycles, sunspots,
maximum entropy method (MEM).",
abstract = "A simple method MEM-MRA, where spectral peaks are located by MEM
(Maximum Entropy Method) and about a dozen most prominent ones are
used in MRA (Multiple Regression Analysis) to estimate their
amplitudes and phases, was applied to the sunspot number (Rz)
series of 1748-1996. Spectral characteristics were different in
the successive 3 intervals of 83 years each. Hence, for
predictions, only data for the recent 83 years were considered
relevant. From the spectra for 1914-1996, the most significant
peaks at 5.3, 8.3, 10.5, 12.2, 47 years were used for
reconstruction. The match between observed and reconstructed
values was good (correlation +0.90). When extrapolated, the
reconstructed values indicate a sunspot number maximum for the
present solar cycle 23 as 140 +/- 9, to occur in year 2000 and for
the next solar cycle 24 as 105 +/- 9, to occur in year
2010-2011.",
issn = "0038-0938 and 1573-093X",
label = "9646",
language = "en",
targetfile = "Prediction of the sunspot maximum of solar cycle 23 by
extrapolation of spectral components.pdf",
urlaccessdate = "05 maio 2024"
}