Magnetic flux braiding: Force-free equilibria and current sheets

被引:39
作者
Longbottom, AW [1 ]
Rickard, GJ
Craig, IJD
Sneyd, AD
机构
[1] Univ St Andrews, Dept Math & Computat Sci, St Andrews KY16 9SS, Fife, Scotland
[2] Univ Waikato, Dept Math, Hamilton, New Zealand
关键词
MHD; plasmas; Sun : corona;
D O I
10.1086/305694
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use a numerical, nonlinear, multigrid magnetic relaxation technique to investigate the generation of current sheets in three-dimensional magnetic flux braiding experiments. We are able to catalog the relaxed nonlinear force-free equilibria resulting from the application of deformations to an initially undisturbed region of plasma containing a uniform vertical magnetic field. The deformations are manifested by imposing motions on the bounding planes to which the magnetic field is anchored. Once imposed, the new distribution of magnetic footpoints are then taken to be fixed, so that the rest of the plasma must then relax to a new equilibrium configuration For the class of footpoint motions that we have examined, we find that singular and nonsingular equilibria can be generated. By singular we mean that within the limits imposed by numerical resolution, we find that there is no convergence to a well-defined equilibrium as the number of grid points in the numerical domain is increased. These singular equilibria contain current "sheets" of ever increasing current intensity and decreasing width; they occur when the footpoint motions exceed a certain threshold and must include both twist and shear in order to be effective. On the basis of these results, we contend that flux braiding will indeed result in significant current generation. We discuss the implications of our results for coronal heating.
引用
收藏
页码:471 / 482
页数:12
相关论文
共 24 条
[1]  
BILLINGHURST MN, 1993, ASTRON ASTROPHYS, V279, P589
[2]   THE SHAPE OF TWISTED, LINE-TIED CORONAL LOOPS [J].
BROWNING, PK ;
HOOD, AW .
SOLAR PHYSICS, 1989, 124 (02) :271-288
[3]   AN INVERSE COORDINATE MULTIGRID METHOD FOR FREE-BOUNDARY MAGNETOHYDROSTATICS [J].
CALLY, PS .
JOURNAL OF COMPUTATIONAL PHYSICS, 1991, 93 (02) :411-425
[4]   NONLINEAR DEVELOPMENT OF THE KINK INSTABILITY IN CORONAL FLUX TUBES [J].
CRAIG, IJD ;
SNEYD, AD .
ASTROPHYSICAL JOURNAL, 1990, 357 (02) :653-661
[5]   A DYNAMIC RELAXATION TECHNIQUE FOR DETERMINING THE STRUCTURE AND STABILITY OF CORONAL MAGNETIC-FIELDS [J].
CRAIG, IJD ;
SNEYD, AD .
ASTROPHYSICAL JOURNAL, 1986, 311 (01) :451-459
[6]  
FIEDLER RAS, 1992, P 1 SOHO WORKSH COR, P73
[7]   Heating and activity of the solar corona .1. Boundary shearing of an initially homogeneous magnetic field [J].
Galsgaard, K ;
Nordlund, A .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A6) :13445-13460
[8]  
Gold T., 1964, NASA SP, V50, P389
[9]   Magnetohydrodynamic turbulence and implications for solar coronal heating [J].
Hendrix, DL ;
VanHoven, G .
ASTROPHYSICAL JOURNAL, 1996, 467 (02) :887-893
[10]  
LONGBOTTOM AW, 1997, UNPUB A AS