A numerical study of thermal convection in a rotating spherical annulus with axial gravitational field by using parametric spline function approximation
DOI10.1108/09615539810226102zbMath0962.76581OpenAlexW2156692242MaRDI QIDQ4700932
S. T. P. T. Srinivas, C. V. Raghava Rao
Publication date: 19 June 2001
Published in: International Journal of Numerical Methods for Heat & Fluid Flow (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1108/09615539810226102
heat fluxBoussinesq fluidtemperature distributionsuniform gravitational fieldconcentric rotating spherescombined convectionparametric spline function approximation
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Cites Work
- A new formulation of the SADI method for the prediction of natural convection flows in cavities
- Convection in a rotating spherical annulus with a uniform axial gravitational field
- Spline function approximation for differential equations
- Thermal convection in rotating spherical annuli - II. Stratified flows
- A note on parametric spline function approximation
- Thermal effects on slow viscous flow between rotating concentric spheres
- NUMERICAL COMPUTATION OF THE NATURAL CONVECTION FLOW ABOUT A HORIZONTAL CYLINDER USING SPLINES
- SPLINE METHOD OF FRACTIONAL STEPS IN NUMERICAL MODEL OF UNSTEADY NATURAL CONVECTION FLOW AT HIGH RAYLEIGH NUMBER
- Axially symmetric motion of a stratified, rotating fluid in a spherical annulus of narrow gap
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