Magnetic field lines for a flux tube

Details Magnetic field lines for a flux tube Magnetic field lines for a flux tube

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..145..197s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 145, no. 1, p. 197-200.

Physics

2

Lines Of Force, Magnetic Field Configurations, Solar Flux, Solar Magnetic Field, Sunspots, Chromosphere, Mathematical Models, Photosphere

Scientific paper

A simple form is found for the magnetic field structure in the neighborhood of a flux tube or sunspot. This model can be used to model various effects, such as solar oscillations in the vicinity of a flux tube. Equations for the magnetic field components in a 2D cylindrically symmetric flux tube equilibrium are derived and solved. The resulting magnetic configuration possesses a strong magnetic field in a thin tube below a reference level (solar photosphere). Above this reference level the field lines spread out in all directions.

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