Detailed_physics_explains_the_fascinating_phenomenon_of_sunspin_and_its_impacts
Measuring this differential rotation isn’t a straightforward task. Early observations relied on tracking sunspots, which are temporary areas of intense magnetic activity on the solar surface. However, sunspots aren’t always evenly distributed across the Sun, introducing potential biases in the measurements. Modern techniques, such as helioseismology – the study of solar oscillations – provide a more accurate and comprehensive picture. Helioseismology allows scientists to probe the Sun’s interior and map its rotation profile in detail. These oscillations are akin to sound waves traveling through the Sun, and their frequencies are affected by the internal rotation rate. This offers a non-invasive method to understand the Sun’s inner workings.
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