Physics of Solar Prominences: II-Magnetic Structure and Dynamics

被引：537
作者：
Mackay, D. H. [1 ]
Karpen, J. T. [2 ]
Ballester, J. L. [3 ]
Schmieder, B. [4 ]
Aulanier, G. [4 ]
机构：
[1] Univ St Andrews, Sch Math & Stat, St Andrews KY16 9SS, Fife, Scotland
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Univ Illes Balears, Dept Fis, Palma De Mallorca 07122, Spain
[4] Observ Paris, LESIA, F-92195 Meudon, Principal, France
来源：
SPACE SCIENCE REVIEWS | 2010年 / 151卷 / 04期
关键词：
Solar magnetic fields; Solar prominences; Oscillations; MHD waves; CONFIGURATIONS SUPPORTING PROMINENCES; FAST MAGNETOHYDRODYNAMIC OSCILLATIONS; FULL-STOKES SPECTROPOLARIMETRY; TWISTED FLUX-TUBE; H-ALPHA; ACTIVE-REGION; FILAMENT CHANNELS; FINE-STRUCTURE; FORCE-FREE; MHD WAVES;
D O I：
10.1007/s11214-010-9628-0
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
引用
收藏
页码：333 / 399
页数：67
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