Modelling coronal magnetic fields

Details Modelling coronal magnetic fields Modelling coronal magnetic fields

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981soph...74..165r&link_type=abstract

(ESA and European Physical Society, ESLAB Symposium on Physics of Solar Variations, 14th, Scheveningen, Netherlands, Sept. 16-19

Physics

12

Solar Corona, Solar Magnetic Field, Stellar Models, Magnetic Dipoles, Magnetic Field Configurations, Solar Wind

Scientific paper

The 'hairy ball' model of coronal magnetic fields has a spherical source
surface separating potential and radial magnetic fields. In the present
model the source surface is chosen such that the wind speed equals the
Alfvenic speed at selected points on the source surface. Results have
been obtained for a dipole base field and an isothermal corona.

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