Magnetic field structures for inverse polarity prominences.

A. O. Schönfelder, A. W. Hood, R. A. S. Fiedler

Research output: Contribution to journalArticlepeer-review


Results of numerical solutions to the equilibrium equation indicate that a fully developed prominence will possess an O-type, but not in general an X-type neutral point.


  • Solar Prominences: Structure
  • Solar Prominences: Numerical Simulations
  • Solar Prominences: Solar Magnetic Fields


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