HR: 1340h
AN: SH53A-1058    [Abstracts]
TI: The Magnetic Structure of X-Ray Bright Points
AU: * DeLuca, E E
EM: edeluca@cfa.harvard.edu
AF: Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138, United States
AU: Van Ballegooijen, A A
EM: avanballegooijen@cfa.harvard.edu
AF: Smithsonian Astrophysical Observatory, 60 Garden St., Cambridge, MA 02138, United States
AU: Harvey, J W
EM: jharvey@noao.edu
AF: National Solar Observatory, BOX 2732 950 N. Cherry Ave., Tuscon, AZ 85726, United States
AU: Henney, C J
EM: chenney@noao.edu
AF: National Solar Observatory, BOX 2732 950 N. Cherry Ave., Tuscon, AZ 85726, United States
AB: 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.
DE: 7509 Corona
DE: 7524 Magnetic fields
DE: 7549 Ultraviolet emissions
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2007 Fall Meeting