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In physics and engineering, the radiative heat transfer from one surface to another is the equal to the difference of incoming and outgoing radiation from the first surface. In general, the heat transfer between surfaces is governed by temperature, surface emissivity properties and the geometry of the surfaces. The relation for heat transfer can be written as an integral equation with boundary conditions based upon surface conditions. Kernel functions can be useful in approximating and solving this integral equation. == Governing equation == The radiative heat exchange depends on the local surface temperature of the enclosure and the properties of the surfaces, but does not depend upon the media. Because media neither absorb, emit, nor scatter radiation. Governing equation of heat transfer between two surface ''A''''i'' and ''A''''j'' : where : : : : : : If the surface of the enclosure is approximated as gray and diffuse surface, and so the above equation can be written as after the analytical procedure : where is the black body emissive power which is given as the function of temperature of the black body : where is the Stefan–Boltzmann constant. 抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Kernel function for solving integral equation of surface radiation exchanges」の詳細全文を読む スポンサード リンク
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