Author/Authors :
D.S. Brown، نويسنده , , C.E. Parnell، نويسنده , , E.E DeLuca، نويسنده , , R.A. McMullen، نويسنده , , L. Golub، نويسنده , , E.R. Priest، نويسنده ,
Abstract :
The three-dimensional magnetic topology of the solar corona is incredibly complex and its effect on the nature of 3D reconnection is profound. We study the supposedly simple topology of a small scale X-ray bright point observed by TRACE and SOHO/MDI, and how it is driven by reconnection when it forms and during the early stages of its lifetime.
