Projects per year
Abstract
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 language | English |
|---|---|
| Pages (from-to) | 333-399 |
| Journal | Space Science Reviews |
| Volume | 151 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - Apr 2010 |
Fingerprint
Dive into the research topics of 'Physics of Solar Prominences: II Magnetic Structure and Dynamics'. Together they form a unique fingerprint.Projects
- 2 Finished
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Solar&Magnetospheric Plasma Theory PP/E1: Solar and Magnetospheric Plasma Theory
Neukirch, T. (PI), Hood, A. (CoI), Parnell, C. (CoI), Priest, E. (CoI), Roberts, B. (CoI) & Wright, A. (CoI)
1/04/07 → 31/03/12
Project: Standard
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PPARC FELOWSHIP-D MACKAY: Dynamic Solar Magnitude Fields
Mackay, D. (PI)
1/10/04 → 30/09/09
Project: Standard
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