Numerical models of quiescent normal polarity prominences

Details Numerical models of quiescent normal polarity prominences Numerical models of quiescent normal polarity prominences

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..141...75f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 141, no. 1, p. 75-90.

Physics

6

Current Sheets, Magnetic Poles, Mathematical Models, Solar Corona, Solar Prominences, Two Dimensional Models, Lorentz Force, Solar Atmosphere, Vertical Orientation

Scientific paper

We present 2D numerical models of quiescent solar prominences with normal magnetic polarity. These models represent an extension to the classical Kippenhahn-Schlueter model in that the prominence is treated as having finite width and height and the external coronal field is matched smoothly to the internal prominence field so that there are no current sheets at the prominence sides. Using typical prominence and coronal values we find solutions to the generalized Grad-Shafranov equation which illustrate the necessary magnetic support. We also discuss some extensions to the basic model.

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