Physical conditions in the reconnection outflow (CROSBI ID 495531)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Skender, Marina ; Vršnak, Bojan ; Martinis, Mladen
engleski
Physical conditions in the reconnection outflow
The amplitude of the standing fast mode shock formed in the reconnection outflow is studied. The dependence on the Mach number of the inflow, the direction of the inflow, the transversal magnetic field, and the plasma to magnetic pressure ratio is investigated in 2-D and 2.5-D model separately. The results are presented stressing the observable quantities such as the band-split of the radio emission excited in the upstream and downstream regions of the fast mode shock. For the range of parameter values appropriate for the occurence of solar flares it is found that the relative band-split should be in the range 10-50%.
reconnection ; MHD
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
Podaci o prilogu
757-760.
2002.
objavljeno
Podaci o matičnoj publikaciji
Solar Variability: From Core to Outer Frontiers
A. Wilson
European Space Agency
92-9092-816-6
Podaci o skupu
The 10th European Solar Physics Meeting
poster
09.09.2002-14.09.2002
Prag, Češka Republika