DocumentCode :
3121173
Title :
One dimensional simulations of MHD shock heating of a stratified solar coronal hole
Author :
Orta, J.A. ; Huerta, M.A. ; Boynton, G.C.
Author_Institution :
University of Miami, Department of Physics, P.O. Box 248046, Coral Gables, Florida 33124, USA
Volume :
2
fYear :
2007
fDate :
17-22 June 2007
Firstpage :
1599
Lastpage :
1604
Abstract :
Our one dimensional numerical simulations describe the evolution of large amplitude Alfvèn waves excited in the lower corona as they travel upwards guided by the open magnetic field lines of a gravitationally stratified solar coronal hole. When the waves reach the region where β ≪ 1 they develop into magnetohydrodynamic (MHD) shocks. The shock waves seem to produce sufficient heat fluxes to be important contributors to the heating of the solar corona.
Keywords :
Corona; Electric shock; Equations; Magnetic fields; Magnetic resonance; Magnetohydrodynamics; Plasma simulation; Plasma temperature; Shock waves; Solar heating;
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Pulsed Power Conference, 2007 16th IEEE International
Conference_Location :
Albuquerque, NM
Print_ISBN :
978-1-4244-0913-6
Electronic_ISBN :
978-1-4244-0914-3
Type :
conf
DOI :
10.1109/PPPS.2007.4652494
Filename :
4652494
Link To Document :
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