Physics of Solar Prominences: II Magnetic Structure and Dynamics

Duncan Hendry Mackay, J Karpen, Jose-Luis Ballester, B Schmieder, G Aulanier

Research output: Contribution to journalArticlepeer-review

403 Citations (Scopus)


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.
Original languageEnglish
Pages (from-to)333-399
JournalSpace Science Reviews
Issue number4
Publication statusPublished - Apr 2010


Dive into the research topics of 'Physics of Solar Prominences: II Magnetic Structure and Dynamics'. Together they form a unique fingerprint.

Cite this