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Tendency of Discreteness of the Solar Amplitude and Intercycle Relatedness

机译:太阳振幅和周期间相关性的离散趋势

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摘要

We suggest that the average of the sunspot number (SSN) over a cycle offers a more appropriate index than the maximum value of the SSN in the evaluation of the activity of solar cycles. We then show that the average SSN has a tendency to take discrete values, that is, integral multiples of 20. This remarkable finding is supported by the fact that SSNs around the maximum are likely to take some particular values. Further, it is shown that there exists a positive correlation in the amplitude between even-numbered cycles and succeeding odd-numbered cycles and an inverse correlation between (2n+1) cycles and (2n+4) cycles wherenrepresents an integer. If these two correlations are combined, it turns out that there exist two mutually independent series of cycles which do not mix or merge.
机译:我们建议,在评估太阳活动周期时,一个太阳黑子数(SSN)的平均值比SSN的最大值提供更合适的指标。然后,我们表明,平均SSN倾向于采用离散值,即20的整数倍。这一惊人发现得到了以下事实的支持:最大值附近的SSN可能采用某些特定值。此外,示出了在偶数周期和随后的奇数周期之间的振幅存在正相关,并且在(2n + 1)个周期和(2n + 4)个周期之间存在反相关,其中n表示整数。如果将这两个相关性组合在一起,那么就会发现存在两个相互独立的循环序列,它们没有混合或合并。

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