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A Relationship Between the Solar Rotation and Activity Analysed by Tracing Sunspot Groups

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Abstract

The sunspot position published in the data bases of the Greenwich Photoheliographic Results (GPR), the US Air Force Solar Optical Observing Network and National Oceanic and Atmospheric Administration (USAF/NOAA), and of the Debrecen Photoheliographic Data (DPD) in the period 1874 to 2016 were used to calculate yearly values of the solar differential-rotation parameters \(A\) and \(B\). These differential-rotation parameters were compared with the solar-activity level. We found that the Sun rotates more differentially at the minimum than at the maximum of activity during the epoch 1977 – 2016. An inverse correlation between equatorial rotation and solar activity was found using the recently revised sunspot number. The secular decrease of the equatorial rotation rate that accompanies the increase in activity stopped in the last part of the twentieth century. It was noted that when a significant peak in equatorial rotation velocity is observed during activity minimum, the next maximum is weaker than the previous one.

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Acknowledgements

The authors wish to thank Hubertus Wöhl for useful sugestions and a careful reading of the manuscript. We acknowledge the staff of the Royal Observatory of Belgium, Brussels, and the staff of the Heliophysical Observatory, Debrecen, Hungary for maintaining and organizing the WDC-SILSO and DPD databases, respectively. This work was partly supported by the Croatian Science Foundation under the project 6212 “Solar and Stellar Variability”, and in part by the University of Rijeka under project number 13.12.1.3.03.

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Correspondence to Domagoj Ruždjak.

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Ruždjak, D., Brajša, R., Sudar, D. et al. A Relationship Between the Solar Rotation and Activity Analysed by Tracing Sunspot Groups. Sol Phys 292, 179 (2017). https://doi.org/10.1007/s11207-017-1199-8

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