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nydus/The Theory of Heat RadiationPublic
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Page 94 of 235
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81.

In calculating the radiant energy which enters the interval (ν,dν) in the time δt on account of reflection from the moving reflector, the rays falling on the reflector at different angles of incidence must be considered separately. Since in the case of a positive v, the frequency is increased by the reflection, the rays which must be considered have, at the time t, the frequency ν1<ν. If we now consider at the time t a monochromatic pencil of frequency (ν1,dν1), falling on the reflector at an angle of incidence θ, a necessary and sufficient condition for its entrance, by reflection, into the interval (ν,dν) is ν=ν1(1+2vcosθc)anddν=dν1(1+2vcosθc). These relations are obtained by substituting ν1 and ν respectively in the equations [eqn:(83)] (83) and [eqn:(86)] (86) in place of the frequencies before and after reflection ν and ν.

The energy which this pencil carries into the interval (ν1,dν) in the time δt is obtained from [eqn:(89)] (89), likewise by substituting ν1 for ν. It is 2𝖪ν1dσcosθdΩdν1(1+2vcosθc)δt=2𝖪ν1dσcosθdΩdνδt. Now we have 𝖪ν1=𝖪ν+(ν1ν)𝖪ν+ where we shall assume 𝖪ν to be finite.

Hence, neglecting small quantities of higher order, 𝖪ν1=𝖪ν2νvcosθc𝖪ν. Thus the energy required becomes 2dσ(𝖪ν2νvcosθc𝖪ν)sinθcosθdθdϕdνδt, and, integrating this expression as above, with respect to dσ, ϕ, and θ, the total radiant energy which enters into the interval (ν,dν) in the time δt becomes 2πF(𝖪ν43νvc𝖪ν)dνδt.\Label[eqn](93)\upshape (93)

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