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A model for quiescent solar prominences with normal polarity

โœ Scribed by A. W. Hood; U. Anzer

Publisher
Springer
Year
1990
Tongue
English
Weight
705 KB
Volume
126
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

A class of 2-D models of solar quiescent prominences, with normal polarity, is presented. These represent an extension to the Kippenhahn-Schlt~ter model for which the prominence configuration matches smoothly onto an external non-potential coronal solution of a constant ~ 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 ill the photosphere.

๐Ÿ“œ SIMILAR VOLUMES

Numerical models of quiescent normal pol
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โœ R. A. S. Fiedler; A. W. Hood ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer ๐ŸŒ English โš– 800 KB

We present 2-D numerical models of quiescent solar prominences with normal magnetic polarity. These models represent an extension to the classical Kippenhahn-Schltiter model in that the prominence is treated as having finite width and height and the external coronal field is matched smoothly to the

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