First slide
Radiation
Question

The plots of spectral radiancy Rλ  versus wave length λ  for three black bodies at  temperatures T1, T2 and T3 respectively are shown.  Their temperatures are such that

Easy
Solution

By Wien’s displacement Law, at maximum intensity  λT= constant. Since 
λ1  <λ3  <  λ2, we can conclude, T1 > T3 > T2.

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