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Numerical methods in convection theory

  • IV. Numerical Solutions
  • Conference paper
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Problems of Stellar Convection

Part of the book series: Lecture Notes in Physics ((LNP,volume 71))

Abstract

Two and three-dimensional computations have enlarged our understanding of nonlinear convection, particularly in Boussinesq fluids. However, we cannot adequately predict the relationship between convective heat transport and the superadiabatic temperature gradient. Nor is there any indication of a preferred length scale, other than the depth of the convecting layer, in a compressible fluid.

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Edward A. Spiegel Jean-Paul Zahn

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© 1977 Springer-Verlag

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Weiss, N.O. (1977). Numerical methods in convection theory. In: Spiegel, E.A., Zahn, JP. (eds) Problems of Stellar Convection. Lecture Notes in Physics, vol 71. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-08532-7_39

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  • DOI: https://doi.org/10.1007/3-540-08532-7_39

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-08532-4

  • Online ISBN: 978-3-540-35982-1

  • eBook Packages: Springer Book Archive

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