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arxiv: 1001.1635 · v1 · pith:DE3ISOSWnew · submitted 2010-01-11 · 🌌 astro-ph.SR

Physics of Solar Prominences: II - Magnetic Structure and Dynamics

D.H. Mackay , J.T. Karpen , J.L. Ballester , B. Schmieder , G. Aulanier This is my paper
classification 🌌 astro-ph.SR
keywords prominencesmodelsobservationsprominencedynamicsformationmagneticresearch
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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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