Abstract
The solar irradiance has been found to change by 0.1% over the recent solar cycle. A change of irradiance of about 0.5% is required to effect the Earth’s climate. How frequently can a variation of this size be expected?
We examine the question of the persistence of non-periodic variations in solar activity. The Hurst exponent, which characterizes the persistence of a time series (Mandelbrot and Wallis, 1969), is evaluated for the series of 14C data for the time interval from about 6000 BC to 1950 AD (Stuiver and Pearson, 1986). We find a constant Hürst exponent, suggesting that solar activity in the frequency range of from 100 to 3000 years includes an important continuum component in addition to the well-known periodic variations. The value we calculate, H ≈ 0.8, is significantly larger than the value of 0.5 that would correspond to variations produced by a white-noise process. This value is in good agreement with the results for the monthly sunspot data reported elsewhere, indicating that the physics that produces the continuum is a correlated random process (Ruzmaikin et al., 1992), and that it is the same type of process over a wide range of time interval lengths.
We conclude that the time period over which an irradiance change of 0.5% can be expected to occur is significantly shorter than that which would be expected for variations produced by a white-noise process.
The full paper has been submitted to Solar Physics. Part of the research decribed here was carried out by JPL, Caltech under a contract with NASA.
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References
Mandelbrot, B., and Wallis, J.: 1969, Water Resources Research 5, 321.
Ruzmaikin, A. A., Feynman, J., and Kosacheva, V. P.: 1992, in Karen L. Harvey (ed.), The Solar Cycle, ASP Conference Series 27, 547.
Stuiver, M., and Pearson, G. W.: 1986, Radiocarbon 28(2B), 805.
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© 1994 Springer Science+Business Media Dordrecht
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Ruzmaikin, A., Feynman, J., Robinson, P. (1994). Long-Term Persistence of Solar Activity. In: Pap, J.M., Fröhlich, C., Hudson, H.S., Tobiska, W.K. (eds) The Sun as a Variable Star: Solar and Stellar Irradiance Variations. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0950-5_47
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DOI: https://doi.org/10.1007/978-94-011-0950-5_47
Publisher Name: Springer, Dordrecht
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