Results 291 to 300 of about 637,772 (329)
Integrated horizontal convective PCR system for clinical diagnostics. [PDF]
Guo W +11 more
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Meltwater from West Antarctic ice sheet tipping affects AMOC resilience. [PDF]
Sinet S, von der Heydt AS, Dijkstra HA.
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AI-powered prediction of hybrid nanofluid dynamics over a cylinder via LM optimized neural network approach. [PDF]
Imran M +5 more
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A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon. [PDF]
Sahu S +9 more
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ZAMM - Journal of Applied Mathematics and Mechanics / Zeitschrift für Angewandte Mathematik und Mechanik, 1973
AbstractThe paper is a study of motions for which the stretching tensor is convected without diffusion. It is shown that the diffusion of the stretching tensor vanishes if and only if the right Cauchy‐Green tensor is equal to its value for a rigid motion plus twice the product of the initial stretching with the elapsed time.
Passman, S. L., Marris, A. W.
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AbstractThe paper is a study of motions for which the stretching tensor is convected without diffusion. It is shown that the diffusion of the stretching tensor vanishes if and only if the right Cauchy‐Green tensor is equal to its value for a rigid motion plus twice the product of the initial stretching with the elapsed time.
Passman, S. L., Marris, A. W.
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CONVECTION | Convection in the Ocean
2003This authoritative resource covers all aspects of atmospheric sciences―including both theory and applications. Nearly 350 articles and over 1,900 figures and photographs are presented, many in full-color. The Encyclopediais an ideal resource for academia, government, and industry in the fields of atmospheric, ocean, and environmental sciences.
Soloviev, Alexander, Klinger, B.
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Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Demarque, Pierre, Robinson, Francis J.
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zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Demarque, Pierre, Robinson, Francis J.
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Solar Convection and Magneto-Convection
1996We explore the general properties of convection in a solar surface layer. Our three-dimensional simulations use a tabulated equation of state that includes excitation and ionization of hydrogen and other abundant atoms, and the formation of H2 molecules. The radiative energy exchange is determined by solving the radiative transfer equation.
Shantanu Basu +3 more
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Convective Plumes in a Convective Field
Journal of the Atmospheric Sciences, 1970Abstract The theory of isolated turbulent plumes given earlier is used to study a field of plumes. Each plume is immersed in the turbulent downdraft which comprises the return flow. The field of flow is specified by three parameters: the heat flux into the atmosphere at the surface, the depth of the convecting layer, and the intensity of turbulence at ...
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Preconditioning convection dominated convection‐diffusion problems
International Journal of Numerical Methods for Heat & Fluid Flow, 1995This paper is concerned with the numerical solution of multi‐dimensional convection dominated convection‐diffusion problems. These problems are characterized by a large parameter, K, multiplying the convection terms. The goal of this work is the development and analysis of effective preconditioners for iteratively solving the large system of linear ...
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