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Dr Kirill Kuzanyan (IZMIRAN, Russia)17/02/2011, 14:00My scientific interests comprise solar and stellar dynamos, their observational manifestations and simple models enabling to reproduce observational data. Thorough analysis of recently available data of systematic ground-based and space-born observational instruments enable us with higher order moments of magnetic field such as helicities. Simple models based of WKB asymptotics within...Go to contribution page
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Mr Jörn Warnecke (Nordita)17/02/2011, 14:30Magnetic buoyancy is believed to drive the transport of magnetic flux tubes from the convection zone to the surface of the Sun. The magnetic fields form twisted loop-like structures in the solar atmosphere. In this paper we use helical forcing to produce a large-scale dynamo-generated magnetic field, which rises even without magnetic buoyancy. A two layer system is used as computational...Go to contribution page
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Dr Rodion Stephanov17/02/2011, 14:50
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Mr Federico STASYSZYN17/02/2011, 15:10We are able to reproduce analitical resultrs from Meinel (1990) of Alfa^2 dynamo in Gadget, an SPH code.Go to contribution page
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