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Titlebook: Dynamo and Dynamics, a Mathematical Challenge; P. Chossat,D. Ambruster,I. Oprea (Faculty of Mathe Book 2001 Springer Science+Business Medi

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Jaya R. Soneji,Madhugiri Nageswara Raot [., ., ., .] and more realistic geometries can be easily studied numerically [6]. However, most flows of liquid metal are fully turbulent before reaching the dynamo threshold: indeed, the magnetic Prandtl number, . = μ.σν, where μ. is the magnetic permeability of vacuum, σ is the electric conducti
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https://doi.org/10.1007/978-3-642-20447-0instability has been studied experimentally by Faller [.] and Caldwell & Van Atta [.], and numerically by Faller & Kaylor [.] , Lilly [.], Melander [.] and Ponty et al. [.]. The linear and nonlinear behaviour of Ekman- Couette instabilities in a plane layer has been discussed by Hoffmann et al. [.].
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Jaya R. Soneji,Madhugiri Nageswara Raold a dynamo? We present eight variations of a flow motivated by the s2t2 flow numerically studied by Dudley and James [.]. Pulse decay measurements of an externally applied magnetic field are used to quantify the approach to transition to dynamo action.
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https://doi.org/10.1007/978-3-642-20447-0 magnetic field, the dielectrophoretic force can be used to produce a central force field under microgravity conditions. In a space experiment, currently under construction, thermal convection in a rotating spherical gap with heated inner sphere and cooled outer sphere will be visualized by a Wollas
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