Confined disruption of a three-dimensional twisted magnetic flux tube

被引:66
作者
Amari, T [1 ]
Luciani, JF
机构
[1] CEA Saclay, Serv Astrophys, DAPNIA,URA 2052, DSM,Ctr Nalt Rech Sci, F-91191 Gif Sur Yvette, France
[2] Ecole Polytech, CNRS, Ctr Phys Theor, F-91128 Palaiseau, France
关键词
MHD; stars : coronae; stars : flare; stars : magnetic fields;
D O I
10.1086/311971
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this Letter, we study the evolution of a magnetic flux tube confined by an overlaying arcade, considering the gradual build up of the twist in the flux tube. During a first stage, the magnetic field evolves quasi-statically through a sequence of force-free equilibria, building up self-helicity (twist) in the flux rope. When a sufficient amount of twist is injected in the system, it cannot reach a neighboring equilibrium and experiences a major disruption in which the magnetic field of the flux tube reconnects with the overlaying arcade. After the relaxation is completed, the configuration remains globally closed and consists of two almost untwisted flux tubes and a closed overlaying arcade. The model might represent a basis for a unified theory of noneruptive and eruptive flares, in which twisted magnetic flux tubes play a crucial role.
引用
收藏
页码:L81 / L84
页数:4
相关论文
共 23 条
[1]   ON SOME PROPERTIES OF FORCE-FREE MAGNETIC-FIELDS IN INFINITE REGIONS OF SPACE [J].
ALY, JJ .
ASTROPHYSICAL JOURNAL, 1984, 283 (01) :349-362
[2]   HOW MUCH ENERGY CAN BE STORED IN A 3-DIMENSIONAL FORCE-FREE MAGNETIC-FIELD [J].
ALY, JJ .
ASTROPHYSICAL JOURNAL, 1991, 375 (02) :L61-L64
[4]  
Amari T, 1996, ASTRON ASTROPHYS, V306, P913
[5]   Very fast opening of a three-dimensional twisted magnetic flux tube [J].
Amari, T ;
Luciani, JF ;
Aly, JJ ;
Tagger, M .
ASTROPHYSICAL JOURNAL, 1996, 466 (01) :L39-+
[6]  
AMARI T, 1999, IN PRESS SIAM SCI CO
[7]  
AMARI T, 1991, ADV SOLAR SYSTEM MAG, P173
[8]  
[Anonymous], 1968, SOL PHYS, DOI DOI 10.1007/BF00155164
[9]  
BADZENKOV S, 1998, APJ, V500, P966
[10]  
Baty H, 1997, ASTRON ASTROPHYS, V318, P621