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RADIANT HEAT TRANSFER
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Thermodynamics Heat Transfer and Fluid Flow Volume 2 of 3
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Radiation Configuration Factor

Heat Transfer RADIATION HEAT TRANSFER Two black  bodies that radiate toward  each other have  a net heat  flux between them.   The net flow rate of heat between them is given by an adaptation of Equation 2-12. Q sA(T 4 1 T42 ) where: A = surface area of the first body (ft2) T1 = temperature of the first body (°R) T2 = temperature of the second body (°R) All bodies above absolute zero temperature radiate some heat.   The sun and earth both radiate heat toward each other.  This seems to violate the Second Law of Thermodynamics, which states that heat cannot flow from a cold body to a hot body.   The paradox is resolved by the fact that each  body must be in direct line  of sight of the other to receive  radiation from it.   Therefore, whenever the cool body is radiating heat to the hot body, the hot body must also be radiating heat to the cool body.  Since the hot body radiates more heat (due to its higher temperature) than the cold body, the net flow of heat is from hot to cold, and the second law is still satisfied. Emissivity Real objects do not radiate as much heat as a perfect black body.   They radiate less heat than a black body and are called gray bodies.   To take into account the fact that real objects are gray bodies, Equation 2-12 is modified to be of the following form. Q esAT 4 where: = emissivity of the gray body (dimensionless) Emissivity  is  simply  a  factor  by  which  we  multiply  the  black  body  heat  transfer  to  take  into account that the black body is the ideal case.   Emissivity is a dimensionless number and has a maximum value of 1.0. Radiation Configuration Factor Radiative  heat  transfer  rate  between  two  gray  bodies  can  be  calculated  by  the  equation  stated below. Q fa  fe    sA(T41 T42 ) Rev. 0 Page 27 HT-02

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