| dbo:abstract |
The Batchelor–Chandrasekhar equation is the evolution equation for the scalar functions, defining the two-point velocity correlation tensor of a homogeneous axisymmetric turbulence, named after George Batchelor and Subrahmanyan Chandrasekhar. They developed the theory of homogeneous axisymmetric turbulence based on Howard P. Robertson's work on isotropic turbulence using an invariant principle. This equation is an extension of Kármán–Howarth equation from isotropic to axisymmetric turbulence. (en) La ecuación de Batchelor-Chandrasekhar es la ecuación de evolución para las funciones escalares, que define el tensor de correlación de velocidad de dos puntos de una turbulencia axisimétrica homogénea, llamada así por George Batchelor y Subrahmanyan Chandrasekhar. Desarrollaron la teoría de la turbulencia asimétrica axial a partir del trabajo de Howard P. Robertson sobre la turbulencia isotrópica utilizando un principio invariante. Esta ecuación es una extensión de la ecuación de Kármán-Howarth de la turbulencia isotrópica con simetría axial. (es) |
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| rdfs:comment |
The Batchelor–Chandrasekhar equation is the evolution equation for the scalar functions, defining the two-point velocity correlation tensor of a homogeneous axisymmetric turbulence, named after George Batchelor and Subrahmanyan Chandrasekhar. They developed the theory of homogeneous axisymmetric turbulence based on Howard P. Robertson's work on isotropic turbulence using an invariant principle. This equation is an extension of Kármán–Howarth equation from isotropic to axisymmetric turbulence. (en) La ecuación de Batchelor-Chandrasekhar es la ecuación de evolución para las funciones escalares, que define el tensor de correlación de velocidad de dos puntos de una turbulencia axisimétrica homogénea, llamada así por George Batchelor y Subrahmanyan Chandrasekhar. Desarrollaron la teoría de la turbulencia asimétrica axial a partir del trabajo de Howard P. Robertson sobre la turbulencia isotrópica utilizando un principio invariante. Esta ecuación es una extensión de la ecuación de Kármán-Howarth de la turbulencia isotrópica con simetría axial. (es) |
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Ecuación de Batchelor-Chandrasekhar (es) Batchelor–Chandrasekhar equation (en) |
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