The structure of active-region magnetic fields - The homogeneous inverse problem

Details The structure of active-region magnetic fields - The homogeneous inverse problem The structure of active-region magnetic fields - The homogeneous inverse problem

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68.1299f&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Nov.-Dec. 1991, p. 1299-1308. In Russian.

Astronomy and Astrophysics

Astronomy

2

Chromosphere, Solar Activity, Solar Magnetic Field, Approximation, Fredholm Equations, Mathematical Models

Scientific paper

Regularization methods are used to determine the structure of a 3D potential magnetic field above the chromosphere on the basis of fibril orientation data and the position of the polarity dividing line. In the potential approximation the problem is reduced to a 1D Fredholm integral equation of the first kind. Existing regularization methods allow this ill-posed problem to be solved. Results of numerical calculations of the model problem are presented.

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