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Influence of desert dust intrusions on ground‐based and satellite‐derived ultraviolet irradiance in southeastern Spain
Author(s) -
Antón M.,
Valenzuela A.,
Román R.,
Lyamani H.,
Krotkov N.,
Arola A.,
Olmo F. J.,
AladosArboledas L.
Publication year - 2012
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 - 10.1029/2012jd018056
Subject(s) - irradiance , environmental science , aerosol , atmospheric sciences , atmosphere (unit) , solar irradiance , satellite , radiometer , ozone monitoring instrument , mineral dust , absorption (acoustics) , meteorology , remote sensing , geology , physics , optics , astronomy
The desert dust aerosols strongly affect propagation of solar radiation through the atmosphere, reducing surface irradiance available for photochemistry and photosynthesis. This paper evaluates effects of desert dust on surface UV erythemal irradiance (UVER), as measured by a ground‐based broadband UV radiometer and retrieved from the satellite Ozone Monitoring Instrument (OMI) at Granada (southern Spain) from January 2006 to December 2010. The dust effects are characterized by the transmittance ratio of the measured UVER to the corresponding modeled clear sky value. The transmittance has an exponential dependency on aerosol optical depth (AOD), with minimum values of ∼0.6 (attenuation of ∼40%). The OMI UVER algorithm does not account for UV aerosol absorption, which results in overestimation of the ground‐based UVER especially during dust episodes with a mean relative difference up to 40%. The application of aerosol absorption post‐correction method reduces OMI bias up to ∼13%. The results highlight great effect of desert dust on the surface UV irradiance in regions like southern Spain, where dust intrusions from Sahara region are very frequent.

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