Physics
Scientific paper
Nov 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nawg.1996..197p&link_type=abstract
Nachr. Akad. Wiss. Göttingen II, Jahrg. 1996, Nr. 4, p. 197 - 201
Physics
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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