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nydus/The Theory of Heat RadiationPublic

This text examines the physical distinction between heat conduction and heat radiation, noting that radiation is independent of the medium through which it passes. It establishes that heat rays are physically identical to light rays and applies the principles of experimental optics to the study of thermal radiation.

Page 120 of 236
Table of Contents

105.

Let us for future use solve also the more general problem of calculating the entropy radiation of a ray consisting of an arbitrary number of plane polarized non-coherent components 𝖪1, 𝖪2, 𝖪3, , the planes of vibration (planes of the electric vector) of which are given by the azimuths ψ1, ψ2, ψ3, . This problem amounts to finding the principal intensities 𝖪0 and 𝖪0 of the whole ray; for the ray behaves in every physical respect as if it consisted of the non-coherent components 𝖪0 and 𝖪0. For this purpose we begin by establishing the value 𝖪ψ of the component of the ray for an azimuth ψ taken arbitrarily. Denoting by f the electric vector of the ray in the direction ψ, we obtain this value 𝖪ψ from the equation f=f1cos(ψ1ψ)+f2cos(ψ2ψ)+f3cos(ψ3ψ)+, where the terms on the right side denote the projections of the vectors of the separate components in the direction ψ, by squaring and averaging and taking into account the fact that f1, f2, f3,  are non-coherent $\mathsf{K}{\psi} &= \mathsf{K}} \cos^{2}(\psi_{1} - \psi) + \mathsf{K{2} \cos^{2}(\psi} - \psi) + \dots \ \LeftText[\qquad]{or} \mathsf{K{\psi} &= A\cos^{2}\psi + B\sin^{2}\psi + C\sin\psi \cos\psi \ \LeftText[\qquad]{where} A &= \mathsf{K}} \cos^{2}\psi_{1} + \mathsf{K{2} \cos^{2}\psi} + \dots \ B &= \mathsf{K{1} \sin^{2}\psi} + \mathsf{K{2} \sin^{2}\psi} + \dots \ C &= 2(\mathsf{K{1} \sin\psi} \cos\psi_{1} + \mathsf{K{2} \sin\psi + \dots).} \cos\psi_{2

\Label[eqn]{(145)}\tag*{\upshape (145)}$

The principal intensities 𝖪0 and 𝖪0 of the ray follow from this expression as the maximum and the minimum value of 𝖪ψ according to the equation d𝖪ψdψ=0or,tan2ψ=CAB. Hence it follows that the principal intensities are $\left.

&𝖪0&𝖪0

\right} = \tfrac{1}{2}(A + B ± \sqrt{(A - B)^{2} + C^{2}}), \Label[eqn]{(146)}\tag*{\upshape (146)}$ or, by taking [eqn:(145)] (145) into account,

$\left.$

&𝖪0&𝖪0

$\right\} = \frac{1}{2}\Biggl(\mathsf{K}_{1} + \mathsf{K}_{2} + \dots \\ ± \sqrt{$

(𝖪1cos2ψ1&+𝖪2cos2ψ2+)2&+(𝖪1sin2ψ1+𝖪2sin2ψ2+)2

}\,\Biggr). \Label[eqn]{(147)}\tag*{\upshape (147)}

Then the entropy radiation required becomes: 𝖫(𝖪0)+𝖫(𝖪0).\Label[eqn](148)\upshape (148)

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