Atmospheric Transmission Beer's Law
Atmospheric Transmission Beer's Law
Atmospheric Transmission Beer's Law
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3/31/10Measuring solar intensity from the ground• We know that the solar irradiance atthe top of the atmosphere (S 0 ) is ofcrucial importance to Earth’s radiationbudget• Satellite sensors now measure thesolar flux and solar spectrum, but howwas this done before the first satellites,using ground-based measurements?• Problem: solar intensity measured atground level is reduced byatmospheric absorption and scattering,but the atmospheric transmittance isunknown. But the latter cannot beinferred without knowing the solar flux– hence a ‘Catch 22’ situation.Measuring solar intensity from the ground• Solution:• Assume a plane-parallel atmosphere with constant properties overthe course of a day (i.e., a clear day with stable temperature,pressure)• For any given wavelength (λ), there are 2 unknowns: the solarintensity (S λ ) and the atmospheric optical depth (τ λ )• From Beer’s <strong>Law</strong>, the intensity of solar radiation measured at sealevel (I λ ) is:µ = cos θ and θ = solar zenith angle23