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Advances in Meteorology
Volume 2012 (2012), Article ID 861026, 14 pages
Synergistic Use of Remote Sensing and Modeling for Tracing Dust Storms in the Mediterranean
1Research and Technology Development Centre, Sharda University, Knowledge Park III, Greater Noida, 201-306, India
2Center for Excellence in Earth Observing, Schmid College of Science and Technology, Chapman University, Orange, CA 92866, USA
3School of Earth and Environmental Sciences, Schmid College of Science and Technology, Chapman University, Orange, CA 92866, USA
4Laboratory of Meteorology, Department of Physics, Athens University, Athens, Greece
5National Balloon Facility, Tata Institute of Fundamental Research, Hyderabad 500 062, India
6Atmospheric Science Section, Oceanography Division, National Remote Sensing Centre, Department of Space-Government of India, Hyderabad 500 625, India
7Department of Physics and Atmospheric Science, Dalhousie University, Halifax, NS, Canada
8Universities Space Research Association, Greenbelt, MD 20770, USA
9NASA Goddard Space Flight Center, Greenbelt, MD 20770, USA
10Department of Environmental Sciences, Faculty of Science, Alexandria University, Moharem Bek, Alexandria 21522, Egypt
Received 17 November 2011; Accepted 17 January 2012
Academic Editor: Achuthan Jayaraman
Copyright © 2012 D. G. Kaskaoutis et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
This study focuses on the detection of the dust source region and monitoring of the transport of the dust plume from its primary outflow to final deposition. The application area is the Sahara desert and the eastern Mediterranean, where two dust events occurred during the period 4–6 February 2009, an unusual event for a winter period. The Aqua-MODIS and OMI observations clearly define the spatial distribution of the dust plumes, while the CALIPSO observations of total attenuated backscatter (TAB) at 532 nm, depolarization ratio (DR), and attenuated color ratio (1064/532 nm) on 5 February 2009 provide a clear view and vertical structure of the dust-laden layer. The dust source region is defined to be near the Chad-Niger-Libyan borders, using satellite observations and model (DREAM) output. This dust plume is vertically extended up to 2.5 km and is observed as a mass plume of dust from surface level to that altitude, where the vertical variation of TAB (0.002 to 0.2) and DR (0.2–0.5) implies dust-laden layer with non-spherical particles. CALIPSO profiles show that after the dust plume reached at its highest level, the dust particles start to be deposited over the Mediterranean and the initial dust plume was strongly attenuated, while features of dust were limited below about 1–1.5 km for latitudes northern of ~36° (Greek territory).
Desert areas are the main sources of aerosols, with the mineral dust comprising more than 35% (1500–2600 Tgyr−1) of the primarily emitted aerosol mass . Elevated dust plumes favor tropospheric heating and modify the temperature profile, while interactions with black carbon aerosols and pollutants alter their physical and chemical properties, such as size distribution, chemical composition, morphology, and hygroscopicity (e.g., [2–10]). Desert dust plays an important role in radiative forcing, with an estimated global mean Top of Atmosphere (TOA) radiative forcing in the range of −0.6 to 0.4 Wm−2 . However, the radiative forcing caused by dust particles is very uncertain in both magnitude and sign [11, 12], mainly triggered by the chemical composition of mineral particles , the wavelength dependence of the dust optical properties , the albedo of the underlying surface , and also the relative height between the dust layer and the clouds . Desert dust can be transported over long distances from the source regions, with the larger particles be deposited near the source, while the smaller ones are suspended in the air for a few days or weeks, thus travelling over large distances .
The Sahara desert is the most important dust source region in the world [17–20]. The occurrence of Saharan dust (SD) events above eastern Mediterranean has a marked seasonal cycle, with a spring maximum and a winter minimum [8, 21–23]. In the summer, dust identification over the region is also frequent due to the longer duration of the dust particles favored by the stable weather conditions, the absence of depressions, and precipitation that favor their wet deposition. Many studies [24, 25] have shown that the Saharan dust events over Mediterranean are mainly driven by the intense cyclones called Sharav, south of the Atlas Mountains (Morocco), mainly during spring and summer. However, depending on the season, various mechanisms for dust outflow and transport are observed under diverse meteorological patterns, plume characteristics, and source regions [24, 25].
Due to the large spatial distribution and the heterogeneous aerosol field over areas affected by dust plumes, the existing ground-based measurements are not capable of monitoring the whole dust cycle, and a combination of ground-based and satellite observations is usually required [26–29]. The MODIS aerosol data (dark target algorithm) have demonstrated their utility for dust monitoring at regional and global scales [30, 31], but they cannot be readily used to identify the dust sources because of difficulties associated with the large albedo over arid surface. The use of TOMS and OMI aerosol Index (AI) presents some promising results for the identification of the dust source regions although its coarse spatial resolution compared to MODIS  presents challenges, while the MODIS new algorithm Deep Blue is capable for aerosol retrievals over land . Finally, CALIPSO profiles, although very useful for the identification of the dust vertical distribution (e.g., [9, 34, 35]), have a very small swath for the overall monitoring of the dust source regions and transport pathways. Therefore, the synergistic use of passive and active remote sensing, along with models (like DREAM) describing the whole dust cycle, provides a new era not only for monitoring the spatial and vertical extend of dust, but also for identifying its source regions.
In the present study, a combination of passive and active satellite retrievals is performed for monitoring the dust cycle in the eastern Mediterranean atmosphere, from its initial outbreak over Sahara to its final dilution and deposition over the Mediterranean Sea and Greece. More specifically, CALIPSO, MODIS, and OMI retrievals are utilized for the detection of the dust source region, the vertical extent of the dust plume, its spatial coverage, and the temporal variability for dust events occurring during the winter period of February 2009. Although the spatial and vertical distribution of dust, as well as its impacts over the Mediterranean has been systematically studied over the years, the main contribution of the present work is the identification of the dust storm region via combined CALIPSO, MODIS, and OMI observations, as well as to provide useful information about their interrelationship in AOD retrievals using the Deep Blue algorithm over land. The satellite observations are also qualitatively compared with model (DREAM) simulations.
2.1. MODIS Retrievals
The two MODIS sensors have widely been used for the identification of the dust in several locations over the globe [12, 26, 29, 33, 36]. MODIS has been acquiring daily global data in 36 spectral bands from visible to thermal infrared (29 spectral bands with 1 km resolution, 5 spectral bands with 500 m resolution, and 2 with 250 m resolution, nadir pixel dimensions) for retrievals of aerosol properties over land and ocean. The data used in this study include Aqua-MODIS aerosol products, that is, AOD550 and Angstrom exponent at 550–865 nm over ocean from Dark Target algorithm  as well as AOD550 over land from the Deep Blue algorithm . Collection 5 (C005, updated to new version 5.1) Aqua-MODIS retrievals were used over the study region (eastern Mediterranean) during the period 4–6 February 2009 with a spatial resolution of 10 × 10 km (Level 2) derived from the MODIS level-2 data.
2.2. CALIPSO Retrievals
The Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) provides new insight in monitoring of atmospheric dust [9, 38–40] by observing the vertical profiles of aerosols and clouds. As part of the NASA A-Train constellation that includes the Aqua, CloudSat, Aura, and PARASOL satellites, CALIPSO has a 98°-inclination orbit and flies at an altitude of 705 km providing daily global maps of the vertical distribution of aerosols and clouds since spring 2006. The CALIPSO payload consists of three instruments: the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP), an Imaging Infrared Radiometer (IIR), and a moderate spatial resolution Wide Field-of-view Camera (WFC). CALIOP provides profiles of backscatter coefficient at 532 and 1064 nm, as well as two orthogonal (parallel and perpendicular) polarization components at 532 nm. The CALIOP can observe aerosol over bright surfaces and beneath thin clouds as well as in clear sky conditions. In the present work we used Level 1B data that contain a half orbit (day or night) of calibrated and geolocated single-shot (highest resolution) lidar profiles, including attenuated backscatter at 532 nm, depolarization ratio (DR) at 532 nm, and attenuated color ratio (ACR) of band 532 nm and 1064 nm. The vertical resolution of the retrievals is 30 m. Retrieving the spatial and optical properties of aerosols and clouds from the CALIPSO backscatter data is confronted by several difficulties that are not faced in the analysis of ground-based lidars. Among these is the very large distance from the target, the high speed at which the satellite traverses the ground track, and the low signal-to-noise ratios that result from the restrictions imposed on space-based platforms. The CALIPSO calibration and uncertainty as well as the CALIOP data products have been documented elsewhere .
2.3. OMI Retrievals
The Aerosol Index (AI) obtained via the Aura-OMI Level-2G (OMTO3, Version 003) with a spatial resolution of 0.25° × 0.25° was used over the study region during the dusty days. AI is a qualitative indicator of near-UV absorbing aerosol particles such as smoke or mineral dust and does not provide indication of sulfate aerosols. The AI is defined as the difference between the measured (including aerosol effects) spectral contrast at the 331 and 360 nm wavelength radiances and the contrast calculated from the radiative transfer theory for a pure molecular (Rayleigh particles) atmosphere . The UV absorbing aerosols (such as smoke and desert dust) produce smaller contrast than predicted by the pure Rayleigh scattering, and they yield positive values, against the near zero or negative ones for the clouds and nonabsorbing aerosols. The AI is especially suitable for detecting the presence of elevated absorbing aerosols above high reflecting surfaces, such as desert and snow/ice, and can also be detected intermingled with clouds and above cloud decks . This concerns great importance regarding the identification of the dust source regions  and in cases when dust plumes are intermingled with clouds. However, the sensitivity of AI to dust aerosols depends strongly on aerosol layer height, while any aerosol below ~1000 m is unlikely to be detected . Recently OMI instrument has gone through row anomalies; therefore, quantitative use of the data has been avoided in the current study.
2.4. DREAM Model Simulations
The integrated modeling system Dust Regional Atmospheric Modeling (DREAM) (http://www.bsc.es/projects/earthscience/DREAM/)  has been widely used for the 3-D simulation of the dust cycle. The model takes into account the major processes of the dust cycle in the atmosphere, from its uplift and advection to wet and dry deposition. The near-surface wind, thermal conditions, and soil features are used for the simulation of the dust production based on the soil moisture, shear-free convection, and turbulent mixing. Furthermore, high-spatial resolution databases including elevation, soil properties, and vegetation cover are included in the model. The model uses 4 categories for dust-particle size, clay, small silt, large silt, and sand with typical radii of 0.73, 6.1, 18, and 38 μm, respectively. The atmospheric lifetime for the first two size bins is larger than ~12 h, and these particles can be transported to long distances whereas the latter 2 are deposited near dust source region. Through continuing development and validation, DREAM has now reached to a high level of dust forecasting able to predict almost all the major dust events over Mediterranean (e.g., [46, 47]).
3.1. Dust Events and Meteorology
The Terra-MODIS true color RGB images, obtained from MODIS surface reflectance product MOD09 (http://modis.gsfc.nasa.gov/data/dataprod/dataproducts.php?MOD_NUMBER=09), during the studied period are shown in Figure 1 covering eastern Mediterranean and surroundings. On the dusty days (4 and 6 February) extensive cloudiness occurred over Greece and the Balkan countries, while the main part of the eastern Mediterranean and Africa was cloudless allowing the dust plumes to be observable. More specifically, on 4 February the dust plume covers the Libyan and Aegean Seas with larger intensity at southern latitudes exhibiting a sharp northwards direction. On the next day some hints of remaining dust are observed over the Bay of Sirti, while the Greek territory is rather clean and cloudless with mean ground measured PM10 mass concentration values of 20 μgm−3 in Athens and AERONET-AOD500 of 0.083 over Crete. However, on 6 February, a new intense dust outbreak started from Algeria desert is joined with another one from Libya and transported towards Greece following a north/northeasterly direction. On that day, the eastern Aegean Sea is free from dust, but is strongly influenced on the next day (not shown). On both days the main dust plumes seem to be transported below the clouds. This is verified from CALIPSO observations showing transport of dust well below 2.5 km, while the cloud base was well above 3–3.5 km. According to the weather report of the National Observatory of Athens, the visibility was limited to a few hundred meters on 4 and 6-7 February in Athens, while 5 February was a day with relative clean sky and good visibility. At midday of 6 February a slight precipitation (0.7 mm) took place over Athens, however, not being able to dilute the dusty atmosphere, which was remained turbid until the evening hours of 7 February when an intense rainfall (29 mm) took place scavenging the dust particles.
The seasonally changed synoptic meteorological conditions over Mediterranean and surrounding continents are the force dynamics for the different air masses affecting the region as well as the outflow, transport pathways, and vertical extent of dust [8, 48, 49]. The meteorological pattern responsible for the present dust outflows is mainly associated with a trough over the Iberian peninsula and a surface cyclone centered over Italy and Adriatic Sea. The result of this atmospheric circulation is a northward flow associated with strong surface and mid-troposphere winds carrying significant amount of dust from Libya over eastern Mediterranean and Greece. It is worth to be noted that the dust outflow on 4 February 2009 covers the same area with those which occurred on 21 February 2001  and 17 April 2005 , indicating similarity in the dust source regions and transport mechanisms. Such meteorological fields favoring dust exposure are more frequent in late winter (although rare) and early spring, since this period favors the depressions above Mediterranean. The duration of such dust events is 1-2 days, since the depressions favoring them are quickly moved and attenuated. They are usually associated with extensive cloud cover over the eastern Mediterranean and Greece, while the dust plume is mainly transported below the clouds (Figure 1). The wind field on the dusty days is shown along with the DREAM dust simulations (Figures 4 and 5).
3.2. Spatial Distribution of Dust Plumes from MODIS and OMI
The spatial distribution of the AOD550 (a) and Angstrom exponent (α550−865) over ocean (b), as obtained from combining retrievals of the Dark Target and Deep Blue algorithms of Aqua-MODIS Level 2 data, is shown in Figure 2 for 4–6 February 2009. The white gaps in MODIS observations correspond to lack of data in Level 2 product due to filters such as cloud contamination.
The high AOD550 values (up to 0.9) clearly indicate the dust plumes that cover Libya, eastern Mediterranean, and Greece on 4 and 6 February, while they are limited over the Bay of Sirti on 5 February. On 4 February, the thick dust plume (high AOD) originated from the coast of Libya, just east of the coastal city of Benghazi. The area just south of the coastal Libyan mountains constitutes a topographic low and was identified as a significant dust source region . The dust plume is transported northward, being substantially thick in southern to Crete areas, while for northern latitudes it attenuates as being diluted by the removal processes. On 5 February the dust plume is limited without affecting Greece, where clean conditions were prevalent. However, these clean conditions lasted for only one day, since on the next day two intense dust plumes: one from Libya and the other from Tunisia, were joined over Ionian Sea affecting Greece on the 6th and 7th February (not shown). Note also the lower AOD values over Sahara desert as detected only from the Deep Blue algorithm compared to those values given over the sea, mainly attributed to the larger uncertainties in the retrievals over bright surfaces. The lower α550−865 values over the oceanic areas affected by dust, although not being so pronounced as the AOD, suggest the presence of coarse-mode particles on the dusty days, while they were higher on the clean day (5 February), with the low α550−865 to be limited in south Mediterranean.
The spatial distribution of OMI-AI is shown in Figure 3 for 4–6 February 2009. The dust plume transported from central to eastern Libya and then over Mediterranean and Greece has a clear signal in AI values (up to 4) on 4 February, in line with the MODIS observations, while on 5 February lower AI values are limited over Libyan desert and coastal-African Mediterranean, suggesting the attenuation of the dust event. Desert dust has usually a direct effect on AI because of its strong dependence on the imaginary part of the refractive index in the UV  and its transportation at elevated layers into the atmosphere. On the other hand, the two new dust plumes observed over Mediterranean on 6 February (MODIS observations) do not show a strong signal on AI (values below 2.5). It is characteristic that the large AI values are observed more northern than 27°N latitude (4 February), while as we will see in the following, the dust source region is detected somewhat southern from that latitude. This fact indicates that in the initial stage of the dust erosion and uplift the AI is rather incapable to allow detection of the event. Dust aerosols transported within the lower boundary layer are easier to be deposited, and their lifetime is much shorter, while in several cases they do not have a clear signal in AI [25, 51]. For these reasons, one cannot simply use the AI values to compare the relative strengths of dust sources in different climate and meteorological regimes; nevertheless, in certain occasions, the AI can provide a rough measure of relative dust concentrations and, hence, relative source strength [8, 19]. In interpreting the results, care has to be taken that some surface effects, such as sea glint and ocean color, can also enhance the AI. Furthermore, AI values over some regions have been removed due to swath overlap resulting in large unrealistic values (see ). Nevertheless, the advantage of AI is that it can be applied over both land and ocean, thus improving the knowledge about the distribution of dust sources and plumes over the globe [16, 53].
3.3. DREAM Simulations
While significant progress has been achieved in characterizing the physical and optical properties as well as the importance of mineral dust in global-scale processes (e.g., [54, 55]), there has been less progress in identifying the environmental processes that affect dust generation in the source regions and the meteorological factors that affect the dust transport and deposition [56–58]. Significant contribution to the latter can be provided by the DREAM model, which is under continuous development by comparing the retrievals (spatially and vertically) with ground-based and satellite measurements . The DREAM results regarding the spatial distribution of the dust loading and concentration are presented in Figures 4(a), 4(b), 5(a), and 5(b), for 4 and 6 February, respectively at 18.00 UTC. Regarding the dust loading, the strong southerly winds are responsible for the transport of significant amount of dust from the eastern Libyan coast towards Mediterranean and Greece (Figure 4(a)). The dust storm seems to originate from south Libya around 25°N and 15°E, which is in agreement with MODIS and OMI observations despite the limitations mentioned above. Over the same area, the dust concentration exhibits its maximum values, while high values (>300 μg m−3) also observed over most part of Greece (Figure 4(b)), continuously decreasing as the dust plume transported away from Africa. On the same day the maximum PM10 concentrations in Athens reached up to 270 μg m−3 comparable to the values predicted by DREAM. The wind field shows that the intense dust storm was driven by the strong southerlies associated with a large trough over Iberian peninsula and northwestern Africa. Two days later, the same system was also active; however, the presence of an anticyclone over Niger and Chad shifted the trough more to the northwest with a major dust plume originating from Algeria and Tunisia and a minor one from Libya (Figures 5(a) and 5(b)). These two were joined in to one over Ionian Sea affecting Greece on 6, and mainly on 7 February (not shown), as it was transported northeastwards. These simulations are also in line with the satellite observations on the same day.
3.4. Vertical Distribution of Dust
Lidar systems on board satellites have been increasingly available in the recent years for aerosol and dust monitoring since the passive satellite sensors are either incapable to give reliable retrievals over bright surfaces, and/or the presence of clouds causes some gaps in the observations; furthermore, these sensors give data only during daytime. On the other hand, the knowledge of dust-aerosol vertical profiles is very crucial as they influence the radiative forcing, heating rate, and stability of the atmosphere [59, 60]. Thus, CALIPSO observations are used to identify the position of the dust and its vertical distribution along the overpass trajectory. During the studied period (4–6 February 2009), CALIPSO overpasses the area in the nighttime and daytime hours of 5 February (Figures 6 and 7). Both figures show the overpass trajectory (moving southwards for nighttime conditions and northwards for daytime) with the vertical profiles of the total attenuated backscatter (TAB) at 532 nm, the attenuated color ratio (ACR) in the 532–1064 nm and the DR. In both figures the presence of clouds is limited over the European continent, so that the dust plume is clearly defined. The hours of the nighttime and daytime overpass (in UTC) are shown below the figures (lower -axis) while the information for the coordinates of the overpass (longitude and latitude) is given above the figure (upper -axis).
3.4.1. Nighttime Overpass
The nighttime overpass of CALIPSO over the area of interest lasts about 6-7 min and crosses the western Balkans, Ionian Sea, Mediterranean, and central Libya. The TAB image shows an extended thick (0.004–0.006 km-1 sr−1) aerosol layer covering most of the satellite track extending up to ~2.5 km. This aerosol layer originated from the south Libyan Desert (~25°N, 15.5°E) near to the Chad and Niger borders. All the CALIPSO nighttime profiles are very characteristic regarding the dust source region since for southern latitudes only few aerosols at elevated layers (3–5 km) are observed. In great consistency, the DREAM simulations highlighted the same area as the dust source region for 4 February (Figure 4). Thus, the nighttime CALIPSO overpass is able to detect the uplift of the dust storm, which starts at the morning hours on 4 February as Terra-MODIS observations shown (Figure 1). The northwards pathway of the dust plume on 4 February, which nearly coincided with the CALIPSO overpass, allows CALIPSO to monitor the whole movement of the dust plume. After its exposure the dust plume is gradually increasing in depth reaching up to 2.5 km in areas ~500 km away from the dust source (over coastal Libya). As the dust layer crosses Mediterranean, its intensity and thickness are gradually decreasing, while its vertical extend is limited to below 2 km with a trend of further decreasing. The CALIPSO profiles indicate that the dust plume has a direct effect on the surface aerosol concentrations. Similarly, DREAM showed (not presented) significant dry dust deposition of ~50–100 μgm−2 over Mediterranean and Greece for the afternoon hours on 4 February 2009.
The vertical extent of the present dust outflow is much lower than those observed over Mediterranean during spring, summer, and autumn [47, 61, 62], where the dust is mainly transported at elevated heights . This may be attributed to the different meteorological conditions prevailing over the area controlling not only the outflow and transport of dust, but also its vertical extend, deposition rates, and lifetime. Thus, in the hot period, the deep mixed layer over Sahara associated with the large convection favors the dust particles to rise up in height, while the absence of intense winds and precipitation favors their longer atmospheric lifetimes and the transport to larger distances. To this respect, studies have found longer duration of dust events over the central and eastern Mediterranean in summer rather than in winter [25, 63].
CALIPSO provides also estimation of the backscatter-related Angstrom exponent between 532 and 1064 nm named ACR or color index or c-ratio, which is mainly related with the particle size and shape. The ACR can present large differences even for the same aerosol type, since based on that Balis et al.  classified the Sahara dust events over Thessaloniki, Greece in three groups with very differing ACR values depending on the intensity of the dust events, the distance from the source region, the deposition of the large particles, the altitude of the dust layer, and mixing with other aerosol types. Ansmann et al.  reported that ACR values below 0.5 are associated with large dust particles, comparable to the values presented in the present dust plume.
The lowermost panel of Figure 6 shows the spatio-temporal variation of the DR, which is defined as the ratio of the perpendicular and parallel components of the attenuated backscatter signal . Its values range from about ~0.014 for a pure molecular atmosphere to ~0.3, or even more, for the presence of nonspherical particles , being a good proxy for spherical and nonspherical aerosol identification. The variations in the DR are due to the detection noise and natural variability of the dust layer. The high values of DR, varying between 0.2 and 0.5 (see Figure 8(a)), indicate the presence of dust with nonspherical particles. Thus, the DR allows inferring the presence of dust over northern Africa and Mediterranean via the large values, which were gradually reduced for northern latitudes due to deposition of the larger dust particles. The observed range of DR and its vertical structure for this specific dust event during February 2009 is consistent with previous values reported over the Sahara region (DR: 0.2 to 0.5) . Similarly, Gobbi et al.  quantified the dust impact on air quality in Rome, Italy based on the high DR values during Sahara dust events. Thus, the vertical profiles of TAB, DR, and ACR, derived from CALIOP high-resolution vertical profiling, are highly useful for studying dust, polluted and dust+polluted aerosols [66, 69].
3.4.2. Daytime Overpass
The daytime CALIPSO overpass (11:58–12:04 UTC) mainly covers a part of the Ionian Sea, western Libyan Sea and eastern continental Libya, approximately 10° eastern from the nighttime overpass for latitudes below 25°N (Figure 7). During the time interval of ~12 hrs between the two CALIPSO overpasses, the dust plume was strongly attenuated over all regions as shown mainly from the TAB image. However, such a conclusion based only on CALIPSO profiles must be avoided due to different overpass tracks for nighttime and daytime conditions, and, therefore, knowledge about the spatial distribution of aerosols is necessary. This can be justified viewing both overpass tracks and the underlying L2 Aqua-MODIS AOD500 (upper left corner), which is large along the nighttime CALIPSO overpass (Bay of Sirti) and low along daytime CALIPSO overpass (Eastern Libya). Thus, a comparison between the CALIPSO observations for revealing the dust attenuation during the 12-hrs interval is not applicable over Africa. In contrast, it can be applicable over the Mediterranean, where the difference between the CALIPSO tracks is below 5° in longitude. This comparison clearly reveals that the dust plume is significantly reduced during the daytime hours of 5 February above the Mediterranean and Greece, as MODIS and OMI showed (Figures 2 and 3).
This suggests that the CALIPSO track on 5 February (nighttime conditions) corresponds to the dust plume that affected eastern Mediterranean on 4 February. According to DREAM, this intense dust outbreak started at the morning hours on 4 February; thus, the fact of presence of thick aerosol layers near the source region about 16-hrs later (CALIPSO nighttime overpass) suggests a strong and continuous uplift of dust. On the other hand, the dust plume was being transported northwards very quickly favored by the intense winds, since Terra-MODIS observes it over Mediterranean during the morning hours on 4 February (Figure 1). Due to low signal-to-noise ratio for daytime lidar observations, the parameters related with aerosol size, shape, and type, that is, ACR and DR, are not clearly present.
3.4.3. Aerosol Profiles according to Latitude
The aerosol properties along the dust transport have been found to exhibit a vertical heterogeneity owing to boundary layer dynamics, altitudinal differences in physical and chemical compositions and dilution and gravitational settling of the particles . Thus, the surface-level characteristics may be different compared to the columnar ones as well as to present considerable differences along the dust transport. In this respect, examining the vertical profiles of aerosols for increasing latitudes along the dust plume is of major importance for understanding the settling of dust particles from the upper levels into the boundary layer as well as the altering of dust aerosol properties after mixing with other aerosols into the atmosphere. The vertical profiles of TAB and DR are plotted for different latitudes along the nighttime and daytime CALIPSO overpasses (Figure 8).
During nighttime, the vertical profiles of backscatter coefficient at 532 nm are strongly dependent on latitude. Near background values are observed for 20°N, which are dramatically increased at 25°N, nearby to the dust source region, for altitudes below 750 hPa (~2.5 km). As the dust plume was transported northward, the surface-level backscatter values decreased and a vertically homogeneous dust layer is observed from the surface to 800 hPa (30°N), which is further attenuated mainly at elevated heights for northern latitudes. The latter suggests gravitational settling of the dust particles from the upper levels into the lower boundary layer as also observed by Colette et al. . The values of about 0.002-0.003 km-1 sr−1 observed at 35°N (over south Greece) are comparable to those reported over Lecce, south Italy during dust events . During daytime the vertical profile is much different for 25°N, with lower values of backscatter due to different CALIPSO overpass track and to attenuation of dust uplift. Also, for 30°N the vertical profile exhibits lower values at elevated heights (except a peak at 800 hPa), while at 35°N large backscatter (~0.006 km-1 sr−1) is shown near the surface probably indicating mixing of deposited dust with anthropogenic aerosols over Greece.
The vertical profiles of the DR during nighttime exhibit large values (~0.3–0.5) over Africa, without any clear dependence on altitude between surface and 750 hPa. Opposite to the backscatter coefficient, DR shows enhanced values also for 20°N, indicating the presence of dust aerosols even for background conditions over Sahara desert, since DR is independent from the aerosol loading . The much lower DR values (~0.1) at 35°N indicate that the concentration of nonspherical dust aerosols was significantly attenuated and the gravitational settling as well as the mixing with anthropogenic aerosols transported from Europe resulted to lower DR. Similarly, Levin et al.  found that the dust particles reaching over Israel were coated by sea-salt and sulfate during their crossing over Mediterranean. On the other hand, the DR profiles during daytime are associated with low signal-to-noise ratio exhibiting unreal peaks and gaps; however, the values at 35° seem to be lower, but near the surface are very large (>1.0), which may be associated with large uncertainties. The combined use of DR and ACR is a proxy for aerosol type identification since Liu et al.  reported values for DR and ACR of ~0.17 (nonsphericity) and 0.8 (coarse particles) for dust occurrence. In the present case, the DR and ACR are higher and lower, respectively, suggesting a thick dust layer.
The overall analysis reveals that CALIPSO profiles may also be used for the dust source identification under certain occasions, in addition to OMI and MODIS data [16, 32]. Furthermore, the synergistic use of these satellite sensors along with MISR multiangle cameras, able to detect aerosols and dust nonsphericity over desert areas , and models predicting the whole atmospheric dust cycle, is essential for monitoring of such phenomena. The identification of major dust sources over the globe will enable us to focus on critical regions and to quantify emission rates and inventories in response to environmental conditions. Such knowledge is essential for the improvement of the global dust models in order to assess the effects of climate change on emissions in the future.
In this paper a synergy of CALIPSO lidar profiles, MODIS and OMI retrievals as well as model DREAM simulations, has been combined to infer the intrusion of Saharan dust over the eastern Mediterranean and Greece during 4–6 February 2009. More specifically, Level 2 Aqua MODIS retrievals for AOD and Angstrom exponent have been used by means of combining Dark Target approach and Deep Blue algorithm (over deserts), in association with L2G OMI-AI values. The CALIPSO data were used to obtain parameters related with aerosol loading, particle size, and shape, that is, attenuated backscatter coefficient at 532, volume depolarization ratio, and attenuated color ratio for nighttime and daytime conditions on 5 February (day and nighttime overpass).
Two intense dust events have been observed over eastern Mediterranean on 4 and 6-7 February 2009, which were well detected by satellites and use of model. CALIPSO and DREAM highlighted the area at ~25°N, 15.5°E in the Libyan Desert as the dust source for the first event on 4 February, while MODIS and OMI observations justified it. After its exposure the dust was uplifted to ~2.5 km and moving northwards affecting eastern Mediterranean and Greece. During the transport pathway the intensity of the dust layer decreased significantly, while its vertical extend was limited to boundary layer, below 1–1.5 km, since the dust particles were deposited over the Mediterranean. The CALIPSO profiles revealed that the dust-aerosol loading and properties exhibited considerable variations depending on the distance from the source and the gravitational settling. Synoptically, the results showed that the vertical aerosol profiles derived from CALIPSO can be considered very useful for the detection of the dust plume, its source region, optical and microphysical characteristics, vertical extent, and modification from its genesis and uplift into the atmosphere to the dilution and deposition at the ground.
The MODIS and CALIPSO scientific teams are gratefully acknowledged for providing high quality satellite data via the Langley Research Center Atmospheric Science Data center. The OMI data were obtained via the Giovanni tool, which is also gratefully acknowledged. The DREAM images for the dusty days were obtained from the Barcelona Super-Computing Center, while the AOD data over Crete from the FORTH-CRETE AERONET station, both highly acknowledged. Authors are thankful to Science System and Applications for financial support to us (AKP, MK). They also thank the scientific and technical staff of the National Observatory of Athens and Ministry of Environment in Greece for providing useful meteorological and atmospheric data.
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