Coronal magnetic fields produced by photospheric shear

Details Coronal magnetic fields produced by photospheric shear Coronal magnetic fields produced by photospheric shear

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cmfp.book.....s&link_type=abstract

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Computer Science

Coronas, Force-Free Magnetic Fields, Photosphere, Shearing, Stellar Magnetic Fields, Dipoles, Free Energy, Magnetic Field Configurations, Potential Fields, Solar Activity

Scientific paper

The magneto-frictional method is used for computing force free fields to examine the evolution of the magnetic field of a line dipole, when there is relative shearing motion between the two polarities. It found that the energy of the sheared field can be arbitrarily large compared with the potential field. It is also found that it is possible to fit the magnetic energy, as a function of shear, by a simple functional form.

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