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Solar Activity Changes During Prolonged Sunspot Minima as Inferred from Indian Monsoon Rainfall Variations

机译:从印度季风降雨变化的推断下,太阳能活动在长期太阳黑子最小值时变化

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We could find a new 5 year periodicity in the occurrences of peaks in sunspot activity and inferred deviations of annual Indian monsoon rainfall variations from the normal during the Maunder minimum (MM) period. This result is explained in terms of solar dynamo functioning in a different mode from normal during the MM where quadrupole field (first harmonic, 5-5.5 years) dominate over dipole field (fundamental, 11 years) causing extreme north south asymmetry in sunspot activity.
机译:我们可以在太阳黑子活动的峰值中找到新的5年性定期,并在最低(MM)期间的正常情况下,年度印度季风降雨变化的推断偏差。在MM在正常运行的情况下,在MM在正常模式(第一次谐波,5-5.5年)占据偶极领域(基本,11年),在偶极领域(基本,11年)在偶像南部不对称的方面,这结果是解释的。

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