North--South Asymmetry in Solar Activity and Solar Cycle Prediction, IV: Prediction for Lengths of Upcoming Solar Cycles
| Autor: | J. Javaraiah |
|---|---|
| Jazyk: | angličtina |
| Rok vydání: | 2019 |
| Předmět: |
Physics
Series (stratigraphy) Sunspot 010504 meteorology & atmospheric sciences Northern Hemisphere FOS: Physical sciences Astronomy and Astrophysics Astrophysics 01 natural sciences Solar cycle Maxima and minima Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science 0103 physical sciences Solar dynamo Maxima 010303 astronomy & astrophysics Southern Hemisphere Solar and Stellar Astrophysics (astro-ph.SR) 0105 earth and related environmental sciences |
| Popis: | We analyzed the daily sunspot-group data reported by the Greenwich Photoheliographic Results (GPR) during the period 1874-1976 and Debrecen Photoheliographic Data (DPD) during the period 1977-2017 and studied North-South asymmetry in the maxima and minima of the Solar Cycles 12-24. We derived the time series of the 13-month smoothed monthly mean corrected whole-spot areas of the sunspot groups in the Sun's whole sphere (WSGA), northern hemisphere (NSGA), and southern hemisphere (SSGA). From these smoothed time series we obtained the values of the maxima and minima, and the corresponding epochs, of the WSGA, NSGA, and SSGA Cycles 12-24. We find that there exists a 44-66 years periodicity in the North-South asymmetry of the minimum. A long periodicity (130-140 years) may exist in the asymmetry of the maximum. A statistically significant correlation exists between the maximum of SSGA Cycle n and the rise time of WSGA Cycle n + 2. A reasonably significant correlation also exists between the maximum of WSGA Cycle n and the decline time of WSGA Cycle n + 2. These relations suggest that the solar dynamo carries memory over at least three solar cycles. Using these relations we obtained the values 11.7 + or - 0.15 years, 11.2 + or - 0.2 years, and 11.45 + or - 0.3 years for the lengths of WSGA Cycles 24, 25, and 26, respectively, and hence, July 2020, October 2031, and March 2043 for the minimum epochs (start dates) of WSGA Cycles 25, 26, and 27, respectively. We also obtained May 2025 and March 2036 for the maximum epochs of WSGA Cycles 25 and 26, respectively. It seems during the late Maunder minimum sunspot activity was absent around the epochs of the maxima of the NSGA-cycles and the minima of the SSGA-cycles, and some activity was present at the epochs of the maxima of some SSGA-cycles and the minima of some NSGA-cycles. 22 pages, 4 tables, 9 figures, to be published in Solar Physics |
| Databáze: | OpenAIRE |
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