Asymmetric structure of an isolated flux arch

Details Asymmetric structure of an isolated flux arch Asymmetric structure of an isolated flux arch

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.208..253z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 208, no. 2, p. 253-260

Physics

Asymmetry, Magnetic Flux, Magnetostatic Fields, Photosphere, Solar Magnetic Field, Solar Physics, Stellar Models, Two Dimensional Models, Boundary Conditions, Chromosphere, Computerized Simulation, Extreme Ultraviolet Radiation, Mathematical Models, Perturbation Theory, Pressure Distribution, Solar Corona

Scientific paper

This paper extends two-dimensional model of symmetric magnetostatic flux arches confined in stratified atmospheres to asymmetric models. Numerical results show that the flux structure is influenced greatly by the boundary condition of magnetic field, the force-free factor, the atmospheric pressure distribution and the position of footprints (especially the width ratio of outlet to entrance, which differs from symmetric case).

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