Pregled bibliografske jedinice broj: 142335
Physical conditions in the reconnection outflow
Physical conditions in the reconnection outflow // Solar Variability: From Core to Outer Frontiers / A. Wilson (ur.).
Prag, Češka Republika: European Space Agency, 2002. str. 757-760 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 142335 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
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 - : European Space Agency, 2002, 757-760
ISBN
92-9092-816-6
Skup
The 10th European Solar Physics Meeting
Mjesto i datum
Prag, Češka Republika, 09.09.2002. - 14.09.2002
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
Ustanove:
Geodetski fakultet, Zagreb,
Institut "Ruđer Bošković", Zagreb
