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10 - Natural Convection

V. Kumaran
Affiliation:
Indian Institute of Science, Bangalore
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Summary

In the analysis of transport at high Peclet number in Chapter 9, it was assumed that the fluid velocity field is specified, and is not affected by the concentration or temperature variations. There are situations, especially in the case of heat transfer, where variations in temperature cause small variations in density, which results in flow in a gravitational field due to buoyancy. Examples of these flows range from circulation in the atmosphere to cooking by heating over a flame. In the former, air heated by the earth's surface rises and cold air higher up in the atmosphere descends due to buoyancy; in the latter, hotter and lighter fluid at the bottom rises due to buoyancy and is replaced by colder and heavier fluid at the top, resulting in significantly enhanced heat transfer.

The heat transfer due to natural convection from heated objects is considered here, and correlations are derived for the Nusselt number as a function of the Prandtl number and the Grashof number. The Prandtl number is the ratio of momentum and thermal diffusion. The Grashof number, defined in Section 2.4 (Chapter 2), is the square of the Reynolds number based on the characteristic fluid velocity generated by buoyancy. In order to determine the heat transfer rate, it is necessary to solve the coupled momentum and energy equations, the former for the velocity field due to temperature variations and the latter for the temperature field. The equations are too complex to solve analytically, and attention is restricted to scaling the equations to determine the relative magnitudes of convection, diffusion and buoyancy. We examine how the dimensionless groups emerge when the momentum and energy equations are scaled, and how these lead to correlations for the Nusselt number. The numerical coefficients in these correlations are not calculated here.

Boussinesq Equations

Consider a heated object with surface temperature T0, in a ambient fluid with temperature T far from the object, as shown in Fig. 10.1 The fluid density is ρ∞ far from the object, but the temperature variation causes a variation in the density near the object. This density variation results in a buoyancy force, which drives the flow.

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Publisher: Cambridge University Press
Print publication year: 2023

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  • Natural Convection
  • V. Kumaran, Indian Institute of Science, Bangalore
  • Book: Fundamentals of Transport Processes with Applications
  • Chapter DOI: https://doi.org/10.1017/9781009036658.011
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  • Natural Convection
  • V. Kumaran, Indian Institute of Science, Bangalore
  • Book: Fundamentals of Transport Processes with Applications
  • Chapter DOI: https://doi.org/10.1017/9781009036658.011
Available formats
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Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

  • Natural Convection
  • V. Kumaran, Indian Institute of Science, Bangalore
  • Book: Fundamentals of Transport Processes with Applications
  • Chapter DOI: https://doi.org/10.1017/9781009036658.011
Available formats
×