The heat-transfer rate per unit area q to a body from a fluid in natural or gravitational convection is a function of the temperature difference

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The heat-transfer rate per unit area q to a body from a fluid in natural or gravitational convection is a function of the temperature difference ΔT, gravity g, body length L, and three fluid properties: kinematic viscosity ν, conductivity k, and thermal expansion coefficient β. Rewrite in dimensionless form if it is known that g and β appear only as the product gβ.

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Establish the variables and their dimensions 9 MT fcn AT L v k 0 LT L LT 10 M... View full answer

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