Shear-Flow Reconnection Causing EUV Bright Point Heating

Details Shear-Flow Reconnection Causing EUV Bright Point Heating Shear-Flow Reconnection Causing EUV Bright Point Heating

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh22a0190b&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH22A-0190

Physics

3210 Modeling, 7507 Chromosphere, 7524 Magnetic Fields, 7835 Magnetic Reconnection, 7843 Numerical Simulation Studies

Scientific paper

EUV/X-ray Bright Points indicate permanent heating processes in the solar atmosphere. We used the information of observed magnetic fields and photospheric motion to simulate numerically by a global MHD approach, coupled to an appropriate kinetic model desrcibing dissipation, the physical processes behind the heating of the solar atmosphere. It appears that shear flow reconnection near the transition region is the main candidate to understand the localized heating behind Bright Points.

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