Transition from the chaotic turbulence to the turbulent structures.
Kingsep, A. (1999)
Discrete Dynamics in Nature and Society
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Displaying similar documents to “Anomalous resistance of the fractal current-carrying corona of Z-pinch.”
Transition from the chaotic turbulence to the turbulent structures.
Rotating shallow water modeling of planetary, astrophysical and plasma vortical structures. (Plasma transport across a magnetic field, model of the Jupiter's GRS, prediction of existence of giant vortices in spiral galaxies).
Nezlin, M.V., Rylov, A.Yu., Snezhkin, E.N., Titishov, K.B., Chernikov, G.P. (1999)
Discrete Dynamics in Nature and Society
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Integrated electrooptic modulators and switches in
Jiří Čtyroký, Rolf Göring, Jiří Janta, Wolfgang Karthe, Andreas Rasch, Mathias Rottschalk, Josef Schröfel (1990)
Kybernetika
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Dissipative nonlinear structures in tokamak plasmas.
Razumova, K.A. (2001)
Discrete Dynamics in Nature and Society
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Combustion in hydraulically resisted flows.
Gregory I. Sivashinsky (2007)
RACSAM
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The effects of hydraulic resistance on premixed gas combustion in tubes and inert porous beds are discussed on the basis of recent research. It is found that the hydraulic resistance causes a gradual precompression and preheating of the unburned gas adjacent to the advancing deflagration which may lead (after an extended induction period) to a localized thermal explosion triggering an abrupt transition from deglagrative to detonative combustion. The hydraulic resistance has a profound...
Numerical simulations in astrophysics: Supernovae explosions, magnetorotational model and neutrino emission.
Bisnovatyi-Kogan, G.S. (1999)
Discrete Dynamics in Nature and Society
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Renormalization group analysis for thermal turbulence.
Riahi, D.N. (1997)
International Journal of Mathematics and Mathematical Sciences
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Dynamic processes during accretion into a black hole.
Bisnovatyi-Kogan, G. S. (2001)
Discrete Dynamics in Nature and Society
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Stellar pulsations and gravitational waves
Kostas Kokkotas (1997)
Banach Center Publications
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Pulsating stars are important sources of information for astrophysics. Nearly every star undergoes some kind of pulsation from the early stages of its formation until the very late ones i.e. the catastrophic creation of a supercompact object (white dwarf, neutron star or black hole). Pulsations of supercompact objects are of great importance for relativistic astrophysics since these pulsations are accompanied by the emission of gravitational radiation. In this review we shall discuss...