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[ascl:1105.007] Sunspot Models

These IDL codes create a thick magneto-static structure with parameters of a typical sunspot in a solar like photosphere - chromosphere. The variable parameters are field strength on the axis, radius, and Wilson depression (displacement of the atmosphere on the axis with respect to the field-free atmosphere). Output are magnetic field vector, pressure and density distributions with radius and height. The structure has azimuthal symmetry. The codes are relatively self explanatory and the download packages contain README files.

Code site:
http://www2.mps.mpg.de/projects/seismo/NA4/MODEL/khomenko.html
Described in:
https://ui.adsabs.harvard.edu/abs/2008ApJ...689.1379K https://ui.adsabs.harvard.edu/abs/2006ApJ...653..739K
Bibcode:
2011ascl.soft05007K

Views: 3923

ascl:1105.007
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