Prediction for the amplitude of solar cycle 24 from the pattern of activity near the cycle minimum |
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Authors: | M. I. Pishkalo |
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Affiliation: | 16166. Astronomical Observatory, National Taras Shevchenko University of Kyiv, ul. Observatornaya 3, Kyiv, 04053, Ukraine
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Abstract: | Correlations are investigated between the pattern of solar activity described by the smoothed monthly relative sunspot numbers (Wolf numbers) near the minimum of a solar cycle and the cycle amplitude. The closest correlation is found between the amplitude of a solar cycle and the sum of the decrease in activity over two years prior to the cycle minimum and the increase in activity over two years after the minimum; the correlation coefficient between these parameters is 0.92. This parameter is used as a precursor to predict the amplitude of solar cycle 24, which is expected to reach its maximum amplitude (85 ± 12) in February 2014. Based on the correlations between the mean parameters of solar cycles, cycle 24 is expected to last for approximately 11.3 years and the minimum of the next cycle 25 is predicted for May 2020. |
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