- Grashof number
The Grashof number mathrm{Gr} is a
dimensionless number influid dynamics andHeat Transfer which approximates the ratio of thebuoyancy toviscous force acting on a fluid. It frequently arises in the study of situations involvingnatural convection . It is named after the German engineerFranz Grashof .:mathrm{Gr}_L = frac{g eta (T_s - T_infty ) L^3}{ u ^2}, for vertical flat plates
:mathrm{Gr}_D = frac{g eta (T_s - T_infty ) D^3}{ u ^2}, for pipes:mathrm{Gr}_D = frac{g eta (T_s - T_infty ) D^3}{ u ^2}, for bluff bodies
where the L and D subscripts indicates the length scale basis for the Grashof Number.
: "g" = acceleration due to Earth's gravity: "β" = volumetric thermal expansion coefficient (equal to approximately 1/T, for ideal fluids, where T is absolute temperature): "T""s" = source temperature: "T""∞" = film temperature: "L" = length: "D" = diameter: "ν" =
kinematic viscosity The transition to turbulent flow occurs in the range 10^8 < mathrm{Gr}_L < 10^9 for natural convection from vertical flat plates. At higher Grashof numbers, the boundary layer is turbulent; at lower Grashof numbers, the boundary layer is laminar.
The product of the Grashof number and the
Prandtl number gives theRayleigh number , a dimensionless number that characterizes convection problems in heat transfer.There is an analogous form of the Grashof number used in cases of natural convection
mass transfer problems.:mathrm{Gr}_c = frac{g eta^* (C_{a,s} - C_{a,a} ) L^3}{ u^2}
where
:eta^* = -frac{1}{ ho} left ( frac{partial ho}{partial C_a} ight )_{T,p}
and
: "g" = acceleration due to Earth's gravity: "C""a,s" = concentration of species "a" at surface: "C""a,a" = concentration of species "a" in ambient medium : "L" = characteristic length: "ν" = kinematic viscosity: "ρ" =
fluid density : "C""a" = concentration of species "a": "T" = constant temperature: "p" = constant pressureee also
References
* Jaluria, Yogesh. "Natural Convection Heat and Mass Transfer" (New York: Pergamon Press, 1980).
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