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This paper presents an analysis of the energy exchange resulting from a 2D steady magnetohydrodynamics (MHD) flow past …
Persistent link: https://www.econbiz.de/10010675993
The bootstrap fraction, I{sub bs}/I{sub p}, and the shape of the bootstrap current density, J{sub bs}(r), can depend sensitively on the shape of the plasma profiles. Beginning with Hirshman`s form for the bootstrap current density, and making a large aspect ratio expansion (proceeding two orders...
Persistent link: https://www.econbiz.de/10009435716
The bootstrap fraction, I{sub bs}/I{sub p}, and the shape of the bootstrap current density, J{sub bs}(r), can depend sensitively on the shape of the plasma profiles. Beginning with Hirshman's form for the bootstrap current density, and making a large aspect ratio expansion (proceeding two orders...
Persistent link: https://www.econbiz.de/10009436175
The effects of the radial electric field E/sub r/ on the bootstrap current in ATF-type configurations are studied with the Drift Kinetic Equation Solver (DKES). It is found that there is a range of E/sub r/ values over which the bootstrap current does not depend on E/sub r/. The effects of E/sub...
Persistent link: https://www.econbiz.de/10009436457
Persistent link: https://www.econbiz.de/10010204668
Persistent link: https://www.econbiz.de/10011795742
In this paper, the effects of variable thermal conductivity and radiation on the flow and heat transfer of an electrically conducting micropolar fluid over a continuously stretching surface with varying temperature in the presence of a magnetic field are considered. The surface temperature is...
Persistent link: https://www.econbiz.de/10010872157
The influence of magnetic fields and cavitation on the Richtmyer–Meshkov (RM) instability in liquid mercury has been studied numerically in 2D geometry. Numerical results shed light on the evolution of the Muon Collider target proposed as a pulsed jet of mercury interacting with high intensity...
Persistent link: https://www.econbiz.de/10010749329
The magnetic field of the Sun displays a periodic behavior known as the solar cycle. The kinematic αΩ dynamo is the standard theoretical model which adequately reproduces the overall features of this magnetic cycle, such as its period and the latitudinal migration of sunspots. We performed...
Persistent link: https://www.econbiz.de/10011059852
In the present comment we point out some errors found in the above referenced paper.
Persistent link: https://www.econbiz.de/10011060868