State the dimensions of emissive power of a perfect blackbody.
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where Ebλ is monochromatic emissive power of a blackbody (W m−2 μm), T is temperature of the body (K), λ is wavelength (μm), C1 is a constant which is 3.74 × 108 W μm4 m−2, and C2 is a constant which is 1.44 × 104 μm K.
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3.01. 4.1 Thermal Radiation.
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