A three-dimensional model for solar prominences

Details A three-dimensional model for solar prominences A three-dimensional model for solar prominences

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...221..326d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 221, no. 2, Sept. 1989, p. 326-337.

Astronomy and Astrophysics

Astrophysics

16

Astronomical Models, Solar Magnetic Field, Solar Prominences, Chromosphere, Convection, Field Strength, Magnetic Field Configurations, Magnetic Flux, Photosphere, Three Dimensional Models

Scientific paper

In an attempt to model the external force field of a prominence, a three-dimensional linear force-free field configuration was studied. The model consists of a fundamental together with a harmonic that is periodic along the prominence. The variation of the prominence height along the prominence is calculated and it is suggested that feet occur where the prominence sags down to low heights.

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