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Communication Dans Un Congrès Année : 2009

Solar prominences

Résumé

Solar filaments (or prominences) are magnetic structures in the corona. They can be represented by twisted flux ropes in a bipolar magnetic environment. In such models, the dipped field lines of the flux rope carry the filament material and parasitic polarities in the filament channel are responsible for the existence of the lateral feet of prominences.
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Dates et versions

hal-03744068 , version 1 (02-08-2022)

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Brigitte Schmieder, Guillaume Aulanier, Tibor Török. Solar prominences. Universal Heliophysical Processes, IAU Symposium 257, Sep 2008, Ionnina, Greece, Greece. pp.223-232. ⟨hal-03744068⟩
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