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The sun can be treated as a blackbody at an effective surface temperature of 10400 R. The sun can be treated as a blackbody a Determine the rate at which infrared radiation energy

The sun can be treated as a blackbody at an effective surface temperature of 10,400 R. The sun can be treated as a blackbody. (a) Determine the rate at which infrared radiation energy (0.76-100 um) is emitted by the sun, in Btu/hft. (b) Determine the fraction of the radiant energy emitted by the sun that falls in the visible range. (c) Determine the wavelength at which the emission of radiation from the sun peaks (d) Calculate and plot the spectral blackbody emissive power E of the sun versus wavelength in the range of 0.01 μm to 1000 μm. Q1: The sun can be treated as a blackbody at an effective surface temperature of 10,400 R. The sun can be treated as a blackbody. (a) Determine the rate at which infrared radiation energy (0.76-100 um) is emitted by the sun, in Btu/hft. (b) Determine the fraction of the radiant energy emitted by the sun that falls in the visible range. (c) Determine the wavelength at which the emission of radiation from the sun peaks (d) Calculate and plot the spectral blackbody emissive power E of the sun versus wavelength in the range of 0.01 μm to 1000 μm.

Jul 31 2020 Read more Less More

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