A model for quiescent solar prominences with normal polarity

Details A model for quiescent solar prominences with normal polarity A model for quiescent solar prominences with normal polarity

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..126..117h&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 126, March 1990, p. 117-133. Research supported by EEC.

Physics

37

Solar Prominences, Stellar Models, Photosphere, Polarity, Solar Magnetic Field

Scientific paper

A class of two-dimensional models of solar quiescent prominences, with normal polarity, is presented. These represent an extension to the Kippenhahn-Schlueter model for which the prominence configuration matches smoothly onto an external nonpotential coronal solution of a constant alpha field. Using typical prominence values, a model is constructed which also matches the coronal conditions. It is found that the magnetic field component along the prominence influences the internal structure of the prominence. A simple extension to the basic models is indicated as a means of taking a lower boundary of the prominence and eliminating parasitic polarities in the photosphere.

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