I. The differential rotation profile of S. Routh et al. – Community of European Solar Radio Astronomers
The phenomenon of differential rotation in the Sun, described by equation 1 where A is the equatorial rotation speed, A and C are latitudinal gradients, and \theta$ is the latitude, is a cornerstone of solar dynamo theory. While helioseismology and feature tracking at optical and EUV wavelengths have helped map this profile at the surface…