Current sheet model of a normal prominence in which the background magnetic lines show a 'dip structure'

Details Current sheet model of a normal prominence in which the background magnetic lines show a 'dip structure' Current sheet model of a normal prominence in which the background magnetic lines show a 'dip structure'

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..154..393l&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 154, no. 2, p. 393-396

Physics

2

Current Sheets, Magnetic Field Configurations, Solar Prominences, Stellar Magnetic Fields, Stellar Models, Two Dimensional Models, Magnetohydrodynamic Stability, Mathematical Models, Solar Corona

Scientific paper

We propose a simple 2D current sheet model of a normal prominence, in
which the lines of the background magnetic field have the 'dip
structure' which seems to be required for such an object to form and to
be stably supported.

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