Title of article :
The Dynamic Evolution of Twisted Magnetic Flux Tubes in a Three-dimensional Convecting Flow. I. Uniformly Buoyant Horizontal Tubes
Author/Authors :
Fan، Y. -G. نويسنده , , Abbett، W. P. نويسنده , , Fisher، G. H. نويسنده ,
Issue Information :
روزنامه با شماره پیاپی 2 سال 2003
Abstract :
The concept of hyperbolic flux tubes (HFTs) is a generalization of the concept of separator field lines for coronal magnetic fields with a trivial magnetic topology. An effective mechanism of a current layer formation in HFTs is proposed. This mechanism is called magnetic pinching, and it is caused by large-scale shearing motions applied to the photospheric feet of HFTs in a way as if trying to twist the HFT. It is shown that in the middle of an HFT such motions produce a hyperbolic flow that causes an exponentially fast growth of the current density in a thin force-free current layer. The magnetic energy associated with the current layer that is built up over a few hours is sufficient for a large flare. Other implications of HFT pinching for solar flares are discussed as well.
Keywords :
magnetic fields , methods: numerical , Sun , Convection , MHD , Sun: interior
Journal title :
Astrophysical Journal
Journal title :
Astrophysical Journal