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Physics of Solar Prominences: II - Magnetic Structure and Dynamics View all abstracts by submitter

Duncan H Mackay   Submitted: 2010-01-13 07:58

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.

Authors: D.H. Mackay, J.T. Karpen, J.L. Ballester, B. Schmieder, G. Aulanier
Projects: None

Publication Status: Accepted, Space Science Reviews
Last Modified: 2010-01-13 15:08
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