Multi-wavelength observations of flares and eruptive filaments

被引：0
|
作者：
Zuccarello, Francesca [1 ]
Contarino, Lidia [2 ]
Romano, Paolo [2 ]
Battiato, Viviana [2 ]
Guglielmino, Salvo L. [1 ]
机构：
[1] Univ Catania, Dipartimento Fis & Astron, Catania, Italy
[2] Osserv Astrofis Catania, INAF, I-95125 Catania, Italy
来源：
ACTA GEOPHYSICA | 2009年 / 57卷 / 01期
关键词：
flares; eruptive filaments; magnetic reconnection; MAGNETIC HELICITY TRANSPORT; TRACE OBSERVATIONS; RECONNECTION; PROMINENCE; MOTIONS; ENERGY; CORONA; MODEL;
D O I：
10.2478/s11600-008-0040-z
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
In this paper we report some results obtained from multi-wavelength observations carried out to study the mechanisms operating in flares and filament eruptions. Most of these studies have given indication of the presence of phenomena that might be considered signatures of magnetic reconnection, while others have pointed out the important role played by magnetic helicity transport in corona before the eruptive phase.
引用
收藏
页码：24 / 30
页数：7
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