The sun's differential rotation pattern has puzzled scientists for decades: While the poles rotate with a period of approximately 34 days, mid-latitudes rotate faster and the equatorial region requires only approximately 24 days for a full rotation.
Long-period oscillations control the sun's differential rotation: Study retrieved 27 March 2024 from https://phys.org/news/2024-03-period-oscillations-sun-differential-rotation.html
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