Physics of Solar Prominences: II - Magnetic Structure and Dynamics

Details Physics of Solar Prominences: II - Magnetic Structure and Dynamics Physics of Solar Prominences: II - Magnetic Structure and Dynamics

2010-01-11

arxiv.org/abs/1001.1635v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

75 pages, 31 pictures, review paper

Scientific paper

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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