Numerical models of quiescent normal polarity prominences

R. A.S. Fiedler*, A. W. Hood

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

9 Citations (Scopus)


We present 2-D numerical models of quiescent solar prominences with normal magnetic polarity. These models represent an extension to the classical Kippenhahn-Schlüter 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 generalised Grad-Shafranov equation which illustrate the necessary magnetic support. We also discuss some extensions to the basic model.

Original languageEnglish
Pages (from-to)75-90
Number of pages16
JournalSolar Physics
Issue number1
Publication statusPublished - 1 Sept 1992


Dive into the research topics of 'Numerical models of quiescent normal polarity prominences'. Together they form a unique fingerprint.

Cite this