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Microphysical and radiative properties of inhomogeneous stratocumulus: Observations and model simulations
Author(s) -
Los A.,
Duynkerke P. G.
Publication year - 2000
Publication title -
quarterly journal of the royal meteorological society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.744
H-Index - 143
eISSN - 1477-870X
pISSN - 0035-9009
DOI - 10.1002/qj.49712657014
Subject(s) - radiative transfer , monte carlo method , effective radius , extinction (optical mineralogy) , marine stratocumulus , liquid water content , radius , atmospheric radiative transfer codes , forward scatter , optical depth , computational physics , single scattering albedo , physics , atmospheric sciences , scattering , environmental science , aerosol , optics , meteorology , astrophysics , cloud computing , statistics , mathematics , computer security , galaxy , computer science , operating system
Detailed microphysical observations made from aircraft during the Atlantic Stratocumulus Transition Experiment are used to examine the optical properties of marine stratocumulus. Special attention is given to the relationship between the droplet size distribution (droplet‐number concentration, effective radius, and liquid‐water content) and the optical extinction parameter. The extinction parameter calculated with measurements from the forward‐scattering spectrometer probe (FSSP) differs only slightly from the extinction parameter obtained from the total droplet spectrum (measured with two optical probes, FSSP and 260X). In contrast, the results for the effective radius and the liquid‐water content show differences up to 40% between the two spectra. A Monte Carlo radiative‐transfer model is initialized with optical properties calculated from the observed microphysics. Monte Carlo simulations of radiative fluxes are in good agreement with observations for well‐mixed boundary‐layer cloud fields.