A two-dimensional model for a solar prominence

Details A two-dimensional model for a solar prominence A two-dimensional model for a solar prominence

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..109..335b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 109, no. 2, 1987, p. 335-349. Research supported by the British and Spanish Ministry of Sci

Computer Science

Numerical Analysis

8

Magnetic Field Configurations, Magnetohydrostatics, Solar Corona, Solar Magnetic Field, Solar Prominences, Two Dimensional Models, Boundary Value Problems, High Temperature, Microstructure, Numerical Analysis

Scientific paper

A two-dimensional magnetohydrostatic model of a vertical prominence sheet is set up by allowing slow variations of the magnetic field and plasma properties with height. The width of the prominence is found to decrease with height and in many cases the field lines become less curved, while the strength of the horizontal magnetic field increases with height, in agreement with observations.

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