Free ConvectionBasic DefinitionsGrashof Number and Rayleigh NumberExampleFree ConvectionA free convection flow field is a self-sustained flow driven by the presence of a temperature gradient. (As opposed to a forced convection flow where external means are used to provide the flow.) As a result of the temperature difference, the density field is not uniform also. Buoyancy will induce a flow current due to the gravitational field and the variation in the density field. In general, a free convection heat transfer is usually much smaller compared to a forced convection heat transfer. It is therefore important only when there is no external flow exists.hotcoldT  Flow is unstable and a circulatorypattern will be induced.Basic DefinitionsBuoyancy effect:Warm, Surrounding fluid, cold, Hot plateNet force=(- gVThe density difference is due to the temperature difference and it can be characterized by ther volumetric thermal expansion coefficient, :1 1 1( )PT T T TT            Grashof Number and Rayleigh NumberDefine Grashof number, Gr, as the ratio between the buoyancy force and the viscous force:332 2( )Sg T T Lg TLGr  • Grashof number replaces the Reynolds number in the convection correlation equation. In free convection, buoyancy driven flow sometimes dominates the flow inertia, therefore, the Nusselt number is a function of the Grashof number and the Prandtle number alone. Nu=f(Gr, Pr). Reynolds number will be important if there is an external flow. (see chapter 11.5, combined forced and free convection.• In many instances, it is better to combine the Grashof number and the Prandtle number to define a new parameter, the Rayleigh number, Ra=GrPr. The most important use of the Rayleigh number is to characterize the laminar to turbulence transition of a free convection boundary layer flow. For example, when Ra>109, the vertical free convection boundary layer flow over a flat plate becomes turbulent.ExampleDetermine the rate of heat loss from a heated pipe as a result of natural (free) convection.Ts=100 CT=0°CD=0.1 mFilm temperature( Tf): averaged boundary layer temperature Tf=1/2(Ts+T )=50 C.kf=0.03 W/m.K, Pr=0.7, =210-5 m2/s, =1/Tf=1/(273+50)=0.0031(1/K)3362 5 21/ 629 /16 8 / 272( )(9.8)(0.0031)(100 0)(0.1)Pr (0.7) 7.6 10 .(2 10 )0.387{0.6 } 26.0 (equation 11.15 in Table 11.1)[1 (0.559 / Pr) ]0.03(26) 7.8( / )0.1( ) (7.8)( )(SDfDSg T T LRaRaNukh Nu W m KDq hA T T          0.1)(1)(100 0) 244.9( )Can be significant if the pipe are long.W