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Physical conditions in the reconnection outflow


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


Naslov
Physical conditions in the reconnection outflow

Autori
Skender, Marina ; Vršnak, Bojan ; Martinis, Mladen

Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni

Izvornik
Solar Variability: From Core to Outer Frontiers / A. Wilson - The Netherlands : European Space Agency, 2002, 757-760

ISBN
92-9092-816-6

Skup
The 10th European Solar Physics Meeting

Mjesto i datum
Prag, Česka, 9. - 14. IX. 2002.

Vrsta sudjelovanja
Poster

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
Reconnection ; MHD

Sažetak
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%.

Izvorni jezik
Engleski

Znanstvena područja
Fizika



POVEZANOST RADA


Projekt / tema
0007017
0098004

Ustanove
Geodetski fakultet, Zagreb,
Institut "Ruđer Bošković", Zagreb