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Velocity fields in and around sunspots at the highest resolution
Proceedings of the International Astronomical Union
AbstractThe flows in and around sunspots are rich in detail. Starting with the Evershed flow along low-lying flow channels, which are cospatial with the horizontal penumbral magnetic fields, Evershed clouds may continue this motion at the periphery of the sunspot as moving magnetic features in the sunspot moat. Besides these well-ordered flows, peculiar motions are found in complex sunspots, where they contribute to the build-up or relaxation of magnetic shear. In principle, thedoi:10.1017/s1743921311015250 fatcat:6635rkgpt5djpkju6wzettdf44