Steady flow models of dark filaments

Details Steady flow models of dark filaments Steady flow models of dark filaments

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....91..129r&link_type=abstract

Astronomy and Astrophysics, vol. 91, no. 1-2, Nov. 1980, p. 129-135.

Physics

20

Filaments, Magnetohydrodynamic Flow, Magnetohydrodynamics, Solar Physics, Solar Prominences, Steady Flow, Chromosphere, Magnetic Field Configurations, Solar Atmosphere, Solar Corona

Scientific paper

Analytic models of dark filaments are constructed using geometries and physical quantities independent of the x-direction, but magnetic and flow vectors having an x-component. The filament has a sharp vertical dip, a small x-component of the magnetic field, and a high velocity coronal condition outside the filament. The filament was correctly simulated by this model on Aug. 7, 1975; the model is based on shock-like transitions between the chromospheric and coronal states with the flow traveling up and coming down to the chromosphere.

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