Problem 4 Emissivity/Absorptivity 0.8 30.6 ་ A white paint that can be used for passive radiative (b) 1 cooling under the Sun. Provided the following simplified spectral absorptivity/emissivity plot (α) or &) on the right, calculate the net radiative heat flux qrad from a uniform-temperature painted surface at Ts=300 K. The Sun's irradiation on Earth is Gsun 1380 W/m² and its blackbody temperature is Tsun = 5800 K. Ignore the radiation from the atmosphere (surroundings). 0.2 0 ° 3 5 DO Wavelength (um)

Principles of Heat Transfer (Activate Learning with these NEW titles from Engineering!)
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Author:Kreith, Frank; Manglik, Raj M.
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Chapter11: Heat Transfer By Radiation
Section: Chapter Questions
Problem 11.49P
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Problem 4
Emissivity/Absorptivity
0.8
30.6
་
A white paint that can be used for passive radiative (b) 1
cooling under the Sun. Provided the following
simplified spectral absorptivity/emissivity plot (α)
or &) on the right, calculate the net radiative heat
flux qrad from a uniform-temperature painted
surface at Ts=300 K. The Sun's irradiation on Earth
is Gsun 1380 W/m² and its blackbody temperature
is Tsun = 5800 K. Ignore the radiation from the
atmosphere (surroundings).
0.2
0
°
3
5
DO
Wavelength (um)
Transcribed Image Text:Problem 4 Emissivity/Absorptivity 0.8 30.6 ་ A white paint that can be used for passive radiative (b) 1 cooling under the Sun. Provided the following simplified spectral absorptivity/emissivity plot (α) or &) on the right, calculate the net radiative heat flux qrad from a uniform-temperature painted surface at Ts=300 K. The Sun's irradiation on Earth is Gsun 1380 W/m² and its blackbody temperature is Tsun = 5800 K. Ignore the radiation from the atmosphere (surroundings). 0.2 0 ° 3 5 DO Wavelength (um)
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