"The Sun's Rotation: Unraveling the Mystery of Long-period Oscillations"

Scientists have discovered a new theory to explain the Sun's differential rotation, which involves long-period oscillations of sound waves in the solar convection zone. These oscillations, detected as swirling motions around the poles, limit the temperature difference between the poles and the equator, ultimately controlling the Sun's bizarre rotation. The relationship between the oscillations and the differential rotation goes both ways, with the oscillations curbing the rotation. This finding could provide insights into the dynamics of other stars as well.