1. Determine numerically the mean value of the photon occupation number for sunlight at wavelengths of 0.5, 1.0, 10, and 100 µm. Assume the sun is a blackbody emitter of temperature 5800 K. For the same wavelengths, determine the mean value of the photon occupation number for a room-temperature blackbody.
1. Determine numerically the mean value of the photon occupation number for sunlight at wavelengths of 0.5, 1.0, 10, and 100 µm. Assume the sun is a blackbody emitter of temperature 5800 K. For the same wavelengths, determine the mean value of the photon occupation number for a room-temperature blackbody.
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Transcribed Image Text:1. Determine numerically the mean value of the photon occupation number for sunlight at
wavelengths of 0.5, 1.0, 10, and 100 µm. Assume the sun is a blackbody emitter of
temperature 5800 K. For the same wavelengths, determine the mean value of the photon
occupation number for a room-temperature blackbody.
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