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Thermal Convection

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Book cover Fluid Dynamics

Part of the book series: Graduate Texts in Physics ((GTP))

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Abstract

Thermal convection is the transport of internal energy by the motion of a fluid. Two types of convection are usually distinguished: free or natural convection and forced convection. Natural convection is a fluid flow whose origin is always a thermal imbalance: it disappears when the temperature gradients vanish.

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Notes

  1. 1.

    Present wording tends to replace the terminology “forced convection” by advection . In this case, temperature is more like a passive scalar and does not, or little, influence the fluid flow.

  2. 2.

    Taking into account their variations with thermodynamic variables would not change the results or the method, but would make the whole derivation more obscure. For this very reason, we shall also neglect the second viscosity ζ.

  3. 3.

    We can make the connection with the coefficient α introduced for the liquids: we have \(\delta \rho /\rho = -\alpha \delta T\), let \(\rho _{1}/\rho _{0} = -\alpha T_{{\ast}}\theta _{1} = -\theta _{1}/\theta _{00}\), therefore \(\alpha = 1/\theta _{00}T_{{\ast}} = 1/T_{l}\).

  4. 4.

    We could, however, approach such a set-up by confining, for example, an oil layer between a layer of mercury in z < 0, and a layer of liquid sodium in z > d!

  5. 5.

    Other solutions may exist where B is not small compared to A, but they are uninteresting for us as we are focusing on the case where A grows first and B follows.

  6. 6.

    We place the boundaries at \(z = \pm \frac{1} {2}\) rather than at z = 0, 1 so as to be able to use the symmetry or the anti-symmetry of the functions with respect to the z = 0 plane.

  7. 7.

    Cahn and Hilliard (1958).

  8. 8.

    This is a metastable chaos.

References

  • Ahlers, G., He, X., Funfschilling, D. & Bodenschatz, E. (2012). Heat transport by turbulent Rayleigh–Bénard convection for Pr ≃ 0.8 and 3 \(\times 10^{12} \lesssim \) Ra \(\lesssim 10^{15}\): Aspect ratio Γ = 0.50. New Journal of Physics, 14(10), 103012.

    Google Scholar 

  • Bejan, A. (1995). Convection heat transfer. New York: Wiley.

    Google Scholar 

  • Bergé, P., Pomeau, Y. & Vidal, C. (1984). Order within chaos. New York: Wiley.

    MATH  Google Scholar 

  • Cahn, J., & Hilliard, J. (1958). Free energy of a non-uniform system I. Interfacial free energy. The Journal of Chemical Physics, 28, 258–267.

    Google Scholar 

  • Chandrasekhar, S. (1961). Hydrodynamic and hydromagnetic stability. Oxford: Clarendon Press.

    MATH  Google Scholar 

  • Chapman, C.J., Proctor, M.R.E. (1980). Nonlinear Rayleigh-Benard convection between poorly conducting boundaries. Journal of Fluid Mechanics, 101, 759–782.

    Article  ADS  MATH  MathSciNet  Google Scholar 

  • Drazin, P. & Reid, W. (1981). Hydrodynamic stability. Cambridge: Cambridge University Press.

    MATH  Google Scholar 

  • Hurle, D., Jakeman, E. & Pike, E. (1966). On the solution of the bénard problem with boundaries of finite conductivity. Proceedings of the Royal Society of London A, 225, 469–475.

    Google Scholar 

  • Niemela, J. J., Skrbek, L., Sreenivasan, K. R. & Donnelly, R. J. (2000). Turbulent convection at very high Rayleigh numbers. Nature, 404, 837–840.

    Article  ADS  Google Scholar 

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Rieutord, M. (2015). Thermal Convection. In: Fluid Dynamics. Graduate Texts in Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-09351-2_7

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