z-logo
open-access-imgOpen Access
Assessment of the African airborne dust mass over the western Mediterranean Sea using Meteosat data
Author(s) -
Dulac François,
Tanré Didier,
Bergametti Gilles,
BuatMénard Patrick,
Desbois Michel,
Sutton David
Publication year - 1992
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/91jd02427
Subject(s) - aerosol , environmental science , atmospheric sciences , radiative transfer , mineral dust , mediterranean sea , aeronet , radiative forcing , air mass (solar energy) , dust storm , mass concentration (chemistry) , remote sensing , optical depth , mediterranean climate , meteorology , physics , geology , geography , optics , archaeology , boundary layer , thermodynamics
The mass of African dust present over the western Mediterranean during a transport episode from northwestern Africa, which occurred in early July 1985, is estimated using a desert aerosol model, an Earth‐atmosphere radiative transfer model and Meteosat visible channel data from 4 days running. Dust pixels are selected from Meteosat images, and their aerosol optical thickness is retrieved. A proportionality factor between aerosol optical thickness and atmospheric columnar aerosol loading is computed and applied to the dust pixels. The total mass of atmospheric particles over the basin is obtained by interpolation and spatial integration. The maximum aerosol optical thickness is 1.8. The maximum aerosol columnar loading is evaluated to be 2.3 g m −2 . The integrated mass of particles present at a given time is estimated to raise up to about 0.6 × 10 12 g at the maximum and the total mass of dust exported from Africa to be of the order of 10 12 g. The method is carefully evaluated and uncertainties are discussed, with particular emphasis on the relationship between atmospheric dust mass and aerosol optical depth. The overall uncertainty on the total mass is roughly a factor ±3. In the absence of clouds it appears that the major uncertainty results from the lack of knowledge of the actual mass‐size distribution of suspended dust particles, pointing out the lack of relevant data on particles larger than 10 μm in diameter. A simple calculation based on results from both computations and simultaneous field measurements yields a net transfer velocity of particles from the dust layer of approximately 1 cm s −1 .

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom