![]() Section II – The development of Planck’s equation is explained as are the all-important fractional functions of the first and second kinds which result when Planck’s equation is integrated between finite limits.Early developments made by experimentalists and theoreticians are examined as they strove to understand the problem of the blackbody. ![]() Section I – Thermal radiation and the blackbody problem are introduced and discussed.Particular attention is paid to the computational aspects employed in the evaluation of these functions together with the various aids developed to facilitate such calculations. ![]() This book gives an account of the development of Planck’s equation together with many of the other functions closely related to it. Today, understanding the behavior of a blackbody is of importance to many fields including thermal and infrared systems engineering, pyrometry, astronomy, meteorology, and illumination. The resulting mathematical form of his law however made working with it a slow and tedious affair. In 1900 the great German theoretical physicist Max Planck formulated a correct mathematical description of blackbody radiation.
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