Inversion method for transmittance of whole atmosphere
A technology of atmospheric transmittance and inversion, applied in the field of atmospheric optics, can solve the problems of less research on atmospheric transmittance
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[0018] According to Bouguer's law, the direct solar radiation E(W / m 2 )for:
[0019] E(λ)=E 0 (λ)·R·exp(-m(θ)·τ(λ))·T g (1)
[0020] where E 0 (λ) is the direct solar spectral irradiance at the last wavelength λ of the atmosphere at a distance of one astronomical unit (AU); R is the sun-earth distance correction factor at the measurement moment (R=(r m / r) 2 , r is the actual distance between the sun and the earth at the time of observation; r m is the average distance between the sun and the earth); m(θ) is the relative air mass (also known as the atmospheric mass number), θ is the solar zenith angle at the observation time; τ(λ) is the total optical thickness of the atmosphere in the vertical direction at the wavelength λ; T g In order to absorb the gas transmittance, in the actual measurement, the measurement wavelength of the general solar pyranometer is selected at the wavelength where the absorption of gas molecules can be ignored, and all T g =1.
[0021] ...
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