Math 2.0

Fluid mechanics Definition

Natural convection

Builds on Convective heat transferTemperature

Definition

Consider a fluid in a gravitational field with acceleration gg, whose density depends on its temperature. Natural convection (or free convection) is convective heat transfer in which the motion of the fluid is caused only by buoyancy forces. These forces arise from density differences due to temperature differences. No flow is imposed from outside, by a pump, a fan, a moving body or a free stream.

Remarks

Example: still air around a hot vertical plate. The air near the plate is warmer and so lighter than the air far away, so it rises along the plate and carries heat away, with no outside forcing.

Non-example: the same plate in the air stream of a fan. The flow is imposed from outside, so this is forced convection. A fluid layer heated from above also shows no natural convection: the warm light fluid is already on top, the layering is stable, and heat moves by conduction only.

In models one often uses the Boussinesq approximation ρ=ρ0(1−β(T−T0))\rho = \rho_0 \big(1 - \beta (T - T_0)\big) in the buoyancy term only, where β\beta is the thermal expansion coefficient. The strength of the buoyant flow is measured by the Grashof number Gr=gβΔTL3/ν2\mathrm{Gr} = g \beta \Delta T L^3 / \nu^2 and the Rayleigh number Ra=GrPr⁡\mathrm{Ra} = \mathrm{Gr} \Pr. Here ΔT\Delta T is a temperature difference, LL a length and ν\nu the kinematic viscosity.

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Further reading

  1. Web https://en.wikipedia.org/wiki/Convection
About this page
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Kinddefinition
WritingW0 stub
MSC76R10, 80A19
DefinesNatural convection
UsesConvective heat transfer, Temperature
Changed3 November 2026

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