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arXiv · 1001.1635

Physics of Solar Prominences: II - Magnetic Structure and Dynamics

D. H. Mackay·J. T. Karpen·J. L. Ballester·B. Schmieder·G. Aulanier
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Abstract

Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.

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D. H. Mackay, J. T. Karpen, J. L. Ballester, B. Schmieder, G. Aulanier. 2010-01-11. Physics of Solar Prominences: II - Magnetic Structure and Dynamics. https://doi.org/10.1007/s11214-010-9628-0

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