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Numerical simulations of a cylinder wake under a strong axial magnetic field

Author
DOUSSET, Vincent1 ; POTHERAT, Alban1
[1] Applied Mathematics Research Centre, Faculty of Engineering and Computing, Coventry University, Priory Street, Coventry CV1 5FB, United Kingdom
Source

Physics of fluids (1994). 2008, Vol 20, Num 1 ; 017104.1-017104.13 ; ref : 43 ref

CODEN
PHFLE6
ISSN
1070-6631
Scientific domain
Mechanics acoustics
Publisher
American Institute of Physics, Melville, NY
Publication country
United States
Document type
Article
Language
English
Keyword (fr)
Allée tourbillon Champ intense Champ magnétique Condition aux limites Conduite rectangulaire Cylindre circulaire Ecoulement MHD Ecoulement conduite Enceinte recyclage Instabilité Kelvin Helmholtz Modélisation Métal liquide Réacteur fusion nucléaire Régime écoulement Sillage Simulation numérique
Keyword (en)
Vortex street High field Magnetic field Boundary condition Rectangular pipe Circular cylinder MHD flow Pipe flow Blanket Kelvin Helmholtz instability Modeling Liquid metal Nuclear fusion reactor Flow regime Wake Numerical simulation
Keyword (es)
Hílera vorticidad Campo intenso Campo magnético Condiciones límites Conducto rectangular Cilindro circular Flujo MHD Flujo conducción Recinto reciclaje Inestabilidad Kelvin Helmholtz Modelización Metal líquido Reactor fusión nuclear Régimen flujo Estela (marina) Simulación numérica
Classification
Pascal
001 Exact sciences and technology / 001D Applied sciences / 001D06 Energy / 001D06D Energy. Thermal use of fuels / 001D06D04 Installations for energy generation and conversion: thermal and electrical energy. / 001D06D04E Controled nuclear fusion plants

Discipline
Energy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
20118230

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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