21. Blackbody radiation: Assuming the object's surface is a flat and Lambertian, the spectral exitance of a blackbody radiator as a function of temperature is given by Planck's formula
21. Blackbody radiation: Assuming the object's surface is a flat and Lambertian, the spectral exitance of a blackbody radiator as a function of temperature is given by Planck's formula
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![21. Blackbody radiation: Assuming the object's surface is a flat and
Lambertian, the spectral exitance of a blackbody radiator as a function of
temperature is given by Planck's formula](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F62cf0025-2a72-406a-bc17-39c2a0537bca%2F90309dc7-711e-4260-81d6-53bc6a6cd64f%2Fzr25xks_processed.png&w=3840&q=75)
Transcribed Image Text:21. Blackbody radiation: Assuming the object's surface is a flat and
Lambertian, the spectral exitance of a blackbody radiator as a function of
temperature is given by Planck's formula
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The spectral exitance of an ideal black body radiation source follows plank's law
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