Journal
SPACE SCIENCE REVIEWS
Volume 151, Issue 4, Pages 333-399Publisher
SPRINGER
DOI: 10.1007/s11214-010-9628-0
Keywords
Solar magnetic fields; Solar prominences; Oscillations; MHD waves
Categories
Funding
- ISSI (Bern)
- European Commission through the European Solar Magnetism Network [HPRN-CT-2002-00313]
- SOLAIRE Network [MTRN-CT-2006-035484]
- Spanish Ministry of Science and Innovation [AYA2006-07637]
- FEDER
- Conselleria de Economia, Hisenda i Innovacio [PCTIB-2005GC3-03]
- UK STFC
- STFC [PP/E001122/1, ST/H001964/1] Funding Source: UKRI
- Science and Technology Facilities Council [PP/E001122/1, ST/H001964/1, PPA/A/S/2003/00045] Funding Source: researchfish
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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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