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Coronal magnetic fields produced by photospheric shear (1987)

Sturrock, P. A. ; Yang, W.-H.

In: CASI

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Publication Date: 2019-06-28

Description: 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.

Keywords: SOLAR PHYSICS

Type: NASA-CR-181514 , NAS 1.26;181514 , CSSA-ASTRO-87-17 , AD-A188691

Format: application/pdf

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