First geometrical pathlengths probability density function derivation of the skylight from spectroscopically highly resolving oxygen A‐band observations: 1. Measurement technique, atmospheric observations and model calculations
- 27 May 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Atmospheres
- Vol. 103 (D10) , 11483-11504
- https://doi.org/10.1029/98jd00725
Abstract
First measurements of the probability density function of geometrical pathlengths (PDF‐GP) for the skylight transmitted from clear and cloudy skies to the terrestrial surface are reported. The measurements are performed using a novel technique, which includes spectroscopically highly resolving observations of the O2 A‐band (760–780 nm) and a Laplacian back transformation of the intensity ratios measured for the set of individual O2 A‐band rotational absorption lines. The technique provides a new and powerful tool to study the radiative transfer (RT) of the atmosphere for different kinds of atmospheric aerosol loadings and cloudiness. First measurements show, as expected, that the photons transmitted by clouds to ground generally experience longer geometrical paths inside the cloud than expected for a corresponding clear sky condition. The comparison of the measured oxygen A‐band absorption system with plane‐parallel discrete ordinate radiative transfer (DISORT) model calculations shows a reasonable agreement for direct Sun and clear sky zenith observations. For cloudy sky the same comparison shows a good agreement between the observed and the modeled weak absorption lines but systematically larger observed than modeled optical densities for strong absorption lines. Our data also suggest that this significant discrepancy is most likely caused by shortcomings in the physical description of the RT by nonstatistical models, which do not properly account for the fractal nature of the terrestrial cloud cover. In particular our study reveals that the photon path statistics involved with the multiple Mie scattering inside clouds is not properly modeled using the DISORT code. Closing this gap in our understanding of the cloud sky RT may possibly provide much of the explanation for the frequently lower modeled than measured cloudy sky absorption of the solar radiation.Keywords
This publication has 34 references indexed in Scilit:
- Optical path modifications due to tropospheric clouds: Implications for zenith sky measurements of stratospheric gasesJournal of Geophysical Research: Atmospheres, 1998
- Observed atmospheric collision‐induced absorption in near‐infrared oxygen bandsJournal of Geophysical Research: Atmospheres, 1998
- Angular dependence of observed reflectances: A comparison with plane parallel theoryJournal of Geophysical Research: Atmospheres, 1997
- Cloud feedback in atmospheric general circulation models: An updateJournal of Geophysical Research: Atmospheres, 1996
- Radiative smoothing in fractal cloudsJournal of Geophysical Research: Atmospheres, 1995
- On the influence of tropospheric clouds on zenith‐scattered‐light measurements of stratospheric speciesGeophysical Research Letters, 1995
- Rotational Raman scattering and the ring effect in zenith‐sky spectraGeophysical Research Letters, 1995
- Multifractal characterizations of nonstationarity and intermittency in geophysical fields: Observed, retrieved, or simulatedJournal of Geophysical Research: Atmospheres, 1994
- The influence of clouds on radiation: A climate‐modeling perspectiveReviews of Geophysics, 1990
- A Method for Determining the Single Scattering Albedo of Clouds Through Observation of the Internal Scattered Radiation FieldJournal of the Atmospheric Sciences, 1981