Green's Function Methods for Potential Magnetic Fields

Details Green's Function Methods for Potential Magnetic Fields Green's Function Methods for Potential Magnetic Fields

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...76..301s&link_type=abstract

Solar Physics, Volume 76, Issue 2, pp.301-321

Physics

118

Scientific paper

The Green's function method to calculate potential magnetic field on the Sun, which was first established by Schmidt (1964) in the case that the field component normal to a flat boundary plane is specified, is extended to the following three cases: (a) The field component along the line of sight, which is not generally normal to the flat boundary plane, is specified; (b) the line of sight component on a spherical boundary surface is specified; (c) the normal component on a spherical surface is specified, together with the condition that the field becomes approximately radial on an outer spherical surface (the so-called source surface). Properties of these Green's functions are examined, and the applicability of these methods to solar magnetic data is discussed.

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