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izvor podataka: crosbi

Physical conditions in the reconnection outflow (CROSBI ID 495531)

Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija

Skender, Marina ; Vršnak, Bojan ; Martinis, Mladen Physical conditions in the reconnection outflow // Solar Variability: From Core to Outer Frontiers / A. Wilson (ur.). European Space Agency, 2002. str. 757-760

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

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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

Povezanost rada

Fizika