Superpenumbral vortex structures.

Physics

Scientific paper

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Sunspots: Magnetohydrodynamics, Sunspots: Gas Motions

Scientific paper

Spectroheliograms in Hα often show vortex structures in the superpenumbral area of sunspots which covers a region from the outer boundary of the spot to about five spot radii. It is possible to find an analytical solution of the magnetohydrodynamic (MHD) basic equations for a special (one dimensional) case of an axisymmetric horizontal layer around a sunspot. Despite its simplicity, this solution reproduces the main facts of the statistical observations and quantitative measurements.

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