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Instead, they display differential rotation; some layers move at different speeds than others. For example, the sun rotates fastest at its equator, slower at increasing latitudes and slowest at ...
The physical origin of this differential rotation is not fully understood. It turns out, long-period solar oscillations discovered in 2021 play a crucial role in controlling the Sun's rotational ...
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Astronomers from the Indian Institute of Astrophysics have mapped the Sun's differential rotation using 100 years of data from the Kodaikanal Solar Observatory. They discovered that the Sun's ...
They have no solid surfaces unlike many planets. The stellar rotation is not constant for all latitudes -- an effect known as differential rotation. It is caused by the fact that hot plasma rises ...
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 ...
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