Abstract
We present a model for quiescent prominences with helical structure. The model is described by two magnetic fields, one produced by photospheric or subphotospheric currents, the other due to currents along the cylindrical model prominence.
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References
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On leave from Max-Planck Institut für Physik und Astrophysik, München.
The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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Anzer, U., Tandberg-Hanssen, E. A model for quiescent prominences with helical structure. Sol Phys 11, 61–67 (1970). https://doi.org/10.1007/BF00156551
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DOI: https://doi.org/10.1007/BF00156551