Abstract

Abstract. Previous studies have provided some insight into the Saharan dust deposition at a few specific locations from observations over long time periods or intensive field campaigns. However, no assessment of the dust deposition temporal variability in connection with its regional spatial distribution has been achieved so far from network observations over more than 1 year. To investigate dust deposition dynamics at the regional scale, five automatic deposition collectors named CARAGA (Collecteur Automatique de Retombées Atmosphériques insolubles à Grande Autonomie in French) have been deployed in the western Mediterranean region during 1 to 3 years depending on the station. The sites include, from south to north, Lampedusa, Majorca, Corsica, Frioul and Le Casset (southern French Alps). Deposition measurements are performed on a common weekly period at the five sites. The mean dust deposition fluxes are higher close to the northern African coasts and decrease following a south–north gradient, with values from 7.4 g m−2 year−1 in Lampedusa (35°31′ N, 12°37′ E) to 1 g m−2 year−1 in Le Casset (44°59′ N, 6°28′ E). The maximum deposition flux recorded is of 3.2 g m−2 wk−1 in Majorca with only two other events showing more than 1 g m−2 wk−1 in Lampedusa, and a maximum of 0.5 g m−2 wk−1 in Corsica. The maximum value of 2.1 g m−2 year−1 observed in Corsica in 2013 is much lower than existing records in the area over the 3 previous decades (11–14 g m−2 year−1). From the 537 available samples, 98 major Saharan dust deposition events have been identified in the records between 2011 and 2013. Complementary observations provided by both satellite and air mass trajectories are used to identify the dust provenance areas and the transport pathways from the Sahara to the stations for the studied period. Despite the large size of African dust plumes detected by satellites, more than 80 % of the major dust deposition events are recorded at only one station, suggesting that the dust provenance, transport and deposition processes (i.e. wet vs. dry) of dust are different and specific for the different deposition sites in the Mediterranean studied area. The results tend to indicate that wet deposition is the main form of deposition for mineral dust in the western Mediterranean basin, but the contribution of dry deposition (in the sense that no precipitation was detected at the surface) is far from being negligible, and contributes 10 to 46 % to the major dust deposition events, depending on the sampling site.

Highlights

  • A reliable estimation of the dust content in the atmosphere and of its variability in space and time is needed to assess desert dust impacts on the Earth system

  • When Moderate Imaging Spectrometer (MODIS) aerosol optical depth (AOD) was unavailable due to cloud cover, we examined the EUMETSAT Monitoring weather and climate from space, Meteosat Second Generation (MSG) Spinning Enhanced Visible and Infrared Imager (SEVIRI) dust false-colour composite product available from ICARE Geo Browse Interface, which gives the opportunity to follow the transport of the dust plume every 15 min (e.g. Schepanski et al, 2007)

  • For each most intense weekly deposition (MID), we identified by using MODIS AOD or MSG satellite observations where dust is coming from

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Summary

Introduction

A reliable estimation of the dust content in the atmosphere and of its variability in space and time is needed to assess desert dust impacts on the Earth system. A validation of the closure of the dust budget in atmospheric dust models needs to quantify precisely the amount of emitted dust, the atmospheric dust load and the dry and wet deposited dust mass (Bergametti and Fôret, 2014). Quantitative estimates of dust emissions in atmospheric models are still affected by large uncertainties (Zender et al, 2004; Textor et al, 2006; Huneeus et al, 2011), mainly because a direct and quantitative validation of soil dust emissions at a large scale remains not possible. Large available data sets of aerosol optical depth (AOD) have been widely and mostly used to validate dust atmospheric contents simulated by 3-D models at global Large available data sets of aerosol optical depth (AOD) have been widely and mostly used to validate dust atmospheric contents simulated by 3-D models at global (e.g. Chin et al, 2002; Ginoux and Torres, 2003; Huneeus et al, 2011) or regional scales (e.g. Cautenet et al, 2000)

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