An Observational Overview of Solar Flares

被引:651
作者
Fletcher, L. [1 ]
Dennis, B. R. [2 ]
Hudson, H. S. [4 ]
Krucker, S. [4 ]
Phillips, K. [5 ]
Veronig, A. [6 ]
Battaglia, M. [1 ]
Bone, L. [5 ]
Caspi, A. [4 ]
Chen, Q. [8 ]
Gallagher, P. [9 ]
Grigis, P. T. [10 ]
Ji, H. [11 ,12 ]
Liu, W. [2 ,13 ]
Milligan, R. O. [3 ]
Temmer, M. [7 ]
机构
[1] Univ Glasgow, Sch Phys & Astron, Astron & Astrophys Grp, Glasgow G12 8QQ, Lanark, Scotland
[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[3] Queens Univ Belfast, Sch Math & Phys, Belfast BT7 1NN, Antrim, North Ireland
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[5] Mullard Space Sci Lab, Dorking RH5 CNT, Surrey, England
[6] Graz Univ, Inst Geophys Astrophys & Meteorol, A-8010 Graz, Austria
[7] Graz Univ, Inst Phys, A-8010 Graz, Austria
[8] Stanford Univ, Dept Phys, Stanford, CA 94305 USA
[9] Trinity Coll Dublin, Sch Phys, Dublin 2, Ireland
[10] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[11] Purple Mt Observ, Nanjing 210008, Peoples R China
[12] New Jersey Inst Technol, Big Bear Solar Observ, Big Bear City, CA 92314 USA
[13] Stanford Lockheed Inst Space Res, Stanford, CA 94305 USA
基金
奥地利科学基金会;
关键词
Sun; HARD X-RAY; CORONAL MASS EJECTIONS; MAGNETIC-FIELD PROPERTIES; HIGH TIME RESOLUTION; LOOP RADIATIVE HYDRODYNAMICS; QUIET ACTIVE REGIONS; WHITE-LIGHT FLARES; GENTLE CHROMOSPHERIC EVAPORATION; ENERGY-RELEASE RATES; PARTICLE-ACCELERATION;
D O I
10.1007/s11214-010-9701-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an overview of solar flares and associated phenomena, drawing upon a wide range of observational data primarily from the RHESSI era. Following an introductory discussion and overview of the status of observational capabilities, the article is split into topical sections which deal with different areas of flare phenomena (footpoints and ribbons, coronal sources, relationship to coronal mass ejections) and their interconnections. We also discuss flare soft X-ray spectroscopy and the energetics of the process. The emphasis is to describe the observations from multiple points of view, while bearing in mind the models that link them to each other and to theory. The present theoretical and observational understanding of solar flares is far from complete, so we conclude with a brief discussion of models, and a list of missing but important observations.
引用
收藏
页码:19 / 106
页数:88
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