Linear force-free fields in the lower corona

Details Linear force-free fields in the lower corona Linear force-free fields in the lower corona

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...56...55b&link_type=abstract

Solar Physics, vol. 56, Jan. 1978, p. 55-66.

Physics

10

Boundary Value Problems, Force-Free Magnetic Fields, Green'S Functions, Solar Corona, Solar Magnetic Field, Boundary Conditions, Dirichlet Problem, Lines Of Force, Neumann Problem

Scientific paper

Boundary conditions are imposed on the normal component of B on two parallel planes which delineate the force-free volume of linear magnetic fields in low coronal levels of the solar atmosphere. Green's function is employed to ensure that equations for the magnetic field energy remain bounded and smooth. Field line tracings of a simple bipolar source distribution are developed and compared with empirical data obtained from visual observations in H(alpha), EUV, and X-rays.

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