Abstract

Extensive lidar measurements of Saharan dust and biomass-burning smoke were performed with one airborne and three ground-based instruments in the framework of the second part of the SAharan Mineral dUst experiMent (SAMUM-2a) during January and February of 2008 at Cape Verde. Further lidar observations with one system only were conducted duringMay and June of 2008 (SAMUM-2b). The active measurements were supported by Sun photometer observations. During winter, layers of mineral dust from the Sahara and biomass-burning smoke from southern West Africa pass Cape Verde on their way to South America while pure dust layers cross the Atlantic on their way to the Caribbean during summer. The mean 500-nm aerosol optical thickness (AOT) observed during SAMUM-2a was 0.35 ± 0.18. SAMUM-2a observations showed transport of pure dust within the lowermost 1.5 km of the atmospheric column. In the height range from 1.5 to 5.0 km, mixed dust/smoke layers with mean lidar ratios of 67 ± 14 sr at 355 and 532 nm, respectively, prevailed. Within these layers, wavelength-independent linear particle depolarization ratios of 0.12–0.18 at 355, 532, and 710 nm indicate a large contribution (30–70%) of mineral dust to the measured optical properties. Ångstr¨om exponents for backscatter and extinction of around 0.7 support this finding. Mean extinction coefficients in the height range between 2 and 4 km were 66 ± 6 Mm−1 at 355 nm and 48 ± 5 Mm−1 at 532 nm. Comparisons with airborne high-spectral-resolution lidar observations show good agreement within the elevated layers. 3–5 km deep dust layers where observed during SAMUM-2b. These layers showed optical properties similar to the ones of SAMUM-1 in Morocco with a mean 500-nm AOT of 0.4 ± 0.2. Dust extinction coefficients were about 80 ± 6 Mm−1 at 355 and 532 nm. Dust lidar ratios were 53 ± 10 sr at 355 and 532 nm, respectively. Dust depolarization ratios showed an increase with wavelength from 0.31 ± 0.10 at 532 nm to 0.37 ± 0.07 at 710 nm.

Highlights

  • Together with sea salt, mineral dust is the most abundant natural aerosol in the Earth’s atmosphere

  • Wandinger et al (2010) applied the observed large effective radii from these SAMUM-1 measurements to explain the discrepancy between the dust lidar ratios of 55 sr at 532 nm that were usually observed during the SAMUM campaigns (Figs 19g and h) and the value of 40 sr used in the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) retrieval (Omar et al, 2009, 2010)

  • We presented lidar measurements performed at Cape Verde in the framework of the second SAMUM experiment

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Summary

Introduction

Mineral dust is the most abundant natural aerosol in the Earth’s atmosphere. The first SAharan Mineral dUst experiMent (SAMUM-1, Heintzenberg, 2009) was conducted in southern Morocco in May and June 2006, to study the microphysical, chemical, optical, and radiative properties of mineral dust aerosol near the source region. The main campaign of SAMUM-2 with the same participants and equipment that proved successful during SAMUM-1 in Morocco was performed at the airport of Praia, Cape Verde (15.0◦N, 23.5◦W, 75 m above sea level, asl) in January and February of 2008 During this time the aerosol layers over Cape Verde originate from the Saharan desert and a belt of strong biomass-burning activity south of the Sahel.

Instrumentation
Sun photometry
Radiosondes
SAMUM-2a Observations
Case studies
Statistical results
SAMUM-2b Observations
Overall findings of the SAMUM campaigns
Summary
Full Text
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