MAXIMUM ENERGY OF SEMI-INFINITE MAGNETIC-FIELD CONFIGURATIONS

被引:192
作者
STURROCK, PA
机构
[1] Ctr. for Space Sci. and Astrophysics, Stanford University, ERL 306, Stanford
关键词
HYDROMAGNETICS; SUN; PARTICLE EMISSION; MAGNETIC FIELDS;
D O I
10.1086/170620
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This article addresses the conjecture by Aly that the maximum-energy state of magnetic field configurations that have a given flux distribution on a given surface is the open-field configuration. We first show that the existence of a maximum-energy configuration depends upon the topology of the source surface: for a multiply connected surface there is no maximum-energy state. However, the magnetic energy is known to be bounded above for a wide class of simply connected surfaces, and we show that in this case there must be a field configuration that has maximum energy. Furthermore, for this configuration the energy is stationary under arbitrary small footpoint displacements that leave the surface flux distribution unchanged. It is then shown that this condition leads to the result that either B(n), the normal component of magnetic field, or j(n), the normal component of current, must vanish at each point on the source surface. This condition is met by the open configuration but not by any other configuration. We discuss the implications of this result for our understanding of flares and of coronal mass ejections.
引用
收藏
页码:655 / 659
页数:5
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