The Magnetic Structure of X-Ray Bright Points

Details The Magnetic Structure of X-Ray Bright Points The Magnetic Structure of X-Ray Bright Points

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh53a1058d&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH53A-1058

Physics

7509 Corona, 7524 Magnetic Fields, 7549 Ultraviolet Emissions

Scientific paper

The magnetic structure of X-Ray Bright Points (XBPs) observed by Hinode, SOLIS and GONG are well represented by potential field extrapolation models. SOLIS observations are used to compare the magnetic field model with X-ray observations. GONG observation allow us to follow the evolution of the magnetic structures that form the XBPs. Detailed examination of the nulls in the corona around the bright points will presented and discussed.

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