The solar constant is defined as the average flux of solar energy incident on the outer fringes
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The solar constant is defined as the average flux of solar energy incident on the outer fringes of the Earth's atmosphere and a commonly used value is \(1.353 \mathrm{~kW} / \mathrm{m}^{2}\). If the Sun has a diameter of \(1.39 \times 10^{6} \mathrm{~km}\) and is assumed to radiate like a black body, what is its effective temperature?
If the Sun is treated as a black body with a temperature of \(5765 \mathrm{~K}\), show that \(99 \%\) of the radiation emitted by the Sun is in the wavelength range 0.25-3.96 \(\mu \mathrm{m}\).
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Advanced Transport Phenomena Analysis Modeling And Computations
ISBN: 9780521762618
1st Edition
Authors: P. A. Ramachandran
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