Chapter 12: Problem 5
What is visible light? How does it differ from the other forms of electromagnetic radiation?
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Chapter 12: Problem 5
What is visible light? How does it differ from the other forms of electromagnetic radiation?
These are the key concepts you need to understand to accurately answer the question.
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Determine the equilibrium temperature of the absorber surface in Prob. 12-98 if the back side of the absorber is insulated.
Solar radiation is incident on the front surface of a thin plate with direct and diffuse components of 300 and \(250 \mathrm{~W} / \mathrm{m}^{2}\), respectively. The direct radiation makes a \(30^{\circ}\) angle with the normal of the surface. The plate surfaces have a solar absorptivity of \(0.63\) and an emissivity of \(0.93\). The air temperature is \(5^{\circ} \mathrm{C}\) and the convection heat transfer coefficient is \(20 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\). The effective sky temperature for the front surface is \(-33^{\circ} \mathrm{C}\) while the surrounding surfaces are at \(5^{\circ} \mathrm{C}\) for the back surface. Determine the equilibrium temperature of the plate.
A small surface of area \(A=3 \mathrm{~cm}^{2}\) emits radiation with an intensity of radiation that can be expressed as \(I_{e}(\theta, \phi)=100 \phi \cos \theta\), where \(I_{e}\) has the units of \(\mathrm{W} / \mathrm{m}^{2} \cdot \mathrm{sr}\). Determine the emissive power from the surface into the hemisphere surrounding it, and the rate of radiation emission from the surface.
A small circular plate with a surface \(A_{1}\) can be approximated as a blackbody. A radiometer with a surface \(A_{2}\) is placed normal to the direction of viewing from the plate at a distance \(L\). Would the irradiation on the radiometer from the plate decrease if the distance \(L\) is doubled, and if so, by how much?
Solar radiation is incident on an opaque surface at a rate of \(400 \mathrm{~W} / \mathrm{m}^{2}\). The emissivity of the surface is \(0.65\) and the absorptivity to solar radiation is \(0.85\). The convection coefficient between the surface and the environment at \(25^{\circ} \mathrm{C}\) is \(6 \mathrm{~W} / \mathrm{m}^{2} \cdot \mathrm{K}\). If the surface is exposed to atmosphere with an effective sky temperature of \(250 \mathrm{~K}\), the equilibrium temperature of the surface is (a) \(281 \mathrm{~K}\) (b) \(298 \mathrm{~K}\) (c) \(303 \mathrm{~K}\) (d) \(317 \mathrm{~K}\) (e) \(339 \mathrm{~K}\)
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