Description
Given aerosol optical depth (AOD), Angstrom alpha and precipitable water (AKA total column water vapor) calculate Linke turbidity factor using Molineaux (1998), Bird-Hulstrom (1980), Berk (1996) and Kasten (1980).
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calculate Angstrom turbidity alpha exponent if not known, from AOD at two wavelengths,
lambda1
andlambda2
:alpha0 = -log(aod1 / aod2) / log(lambda1 / lambda2)
Example with
lambda1 = 1240nm
andlambda2 = 550nm
alpha0 = -log(aod1240nm / aod550nm) / log(1240 / 550)
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get
aod
at 700[nm] fromalpha
aod700 = aod550* ((700 / 550) ^ (-alpha0))
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From numerically integrated spectral simulations done with Modtran (Berk, 1996), Molineaux (1998) obtained for the broadband optical depth of a clean and dry atmopshere (fictious atmosphere that comprises only the effects of Rayleigh scattering and absorption by the atmosphere gases other than the water vapor) the following expression where
M
is airmass.delta_cda = - 0.101 + 0.235 * M ^ (-0.16)
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The broadband water vapor optical depth where
pwat
is the precipitable water vapor content of the atmosphere in [cm]. The precision of these fits is better than 1% when compared with Modtran simulations in the range 1 < M < 6 and 0 < w < 5 cm.delta_w = 0.112 * M ^ (-0.55) * pwat ^ (0.34);
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Aerosol
either using (Molineaux 1998)
delta_a = aod700
or using (Bird-Hulstrom 1980)
delta_a = 0.27583*aod380 + 0.35*aod500
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Using the Kasten pyrheliometric formula (1980), the Linke turbidity at M
TL = -(9.4 + 0.9*M) * log(exp(-M * (delta_cda + delta_w + delta_a))) / M
This derivation was developed in collaboration with Armel Oumbe @aoumbe
references: