Remote sensing of NO2
Blackbody radiation 1
Type the missing terms into the gaps in the equation for Planck's Law.
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E
λ
_  = 
2 _ _
_

λ
_
exp
_

_ λ
_

where

Eλ monochromatic irradiance [W·m-2·m-1]
λ wavelength [m]
h Planck's constant, 6.6260755(40) 6•10–34 [J·s]
k Boltzmann's constant, 1.380 658(12)•10–23 [J·K–1]
c speed of light, 2.99792458·108 [m·s-1]
T temperature [K]
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