Title of article
Magnetic structure and reconnection of x-ray bright points in the solar corona Original Research Article
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 ,
Issue Information
دوهفته نامه با شماره پیاپی سال 2002
Pages
7
From page
1093
To page
1099
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.
Journal title
Advances in Space Research
Serial Year
2002
Journal title
Advances in Space Research
Record number
1127964
Link To Document