Atmos. Meas. Tech., 10, 4439–4457, 2017 https://doi.org/10.5194/amt-10-4439-2017 © Author(s) 2017. This work is distributed under the Creative Commons Attribution 4.0 License. Comparative assessment of GRASP algorithm for a dust event over Granada (Spain) during ChArMEx-ADRIMED 2013 campaign Jose A. Benavent-Oltra1,2, Roberto Román1,2, María J. Granados-Muñoz1,2, Daniel Pérez-Ramírez1,2, Pablo Ortiz-Amezcua1,2, Cyrielle Denjean3, Anton Lopatin4, Hassan Lyamani1,2, Benjamin Torres4,5, Juan L. Guerrero-Rascado1,2, David Fuertes5, Oleg Dubovik4, Anatoli Chaikovsky6, Francisco J. Olmo1,2, Marc Mallet3, and Lucas Alados-Arboledas1,2 1Department of Applied Physics, University of Granada, 18071 Granada, Spain 2Andalusian Institute for Earth System Research (IISTA-CEAMA), University of Granada, Autonomous Government of Andalusia, 18006 Granada, Spain 3CNRM, Centre National de la Recherche Météorologique (UMR3589, CNRS, Météo-France), Toulouse, France 4Laboratoire d’Optique Atmosphérique, Université de Lille 1, Villeneuve d’Ascq, France 5GRASP-SAS, Remote sensing developments, LOA/Université Lille-1, Villeneuve d’Ascq, France 6Institute of Physics, National Academy of Science, Minsk, Belarus Correspondence to: Jose A. Benavent-Oltra (
[email protected]) Received: 19 June 2017 – Discussion started: 4 July 2017 Revised: 21 September 2017 – Accepted: 13 October 2017 – Published: 17 November 2017 Abstract. In this study, vertical profiles and columnintegrated aerosol properties retrieved by the GRASP (Generalized Retrieval of Atmosphere and Surface Properties) algorithm are evaluated with in situ airborne measurements made during the ChArMEx-ADRIMED field campaign in summer 2013. In the framework of this campaign, two different flights took place over Granada (Spain) during a desert dust episode on 16 and 17 June. The GRASP algorithm, which combines lidar and sun–sky photometer data measured at Granada, was used to retrieve aerosol properties. Two sun-photometer datasets are used: one co-located with the lidar system and the other in the Cerro Poyos station, approximately 1200 m higher than the lidar system but at a short horizontal distance. Column-integrated aerosol microphysical properties retrieved by GRASP are compared with AERONET products showing a good agreement. Differences between GRASP retrievals and airborne extinction profiles are in the range of 15 to 30%, depending on the instrument on board the aircraft used as reference. On 16 June, a case where the dust layer was coupled to the aerosol layer close to surface, the total volume concentration differences between in situ data and GRASP retrieval are 15 and 36% for Granada and Cerro Poyos retrievals, respectively. In contrast, on 17 June the dust layer was decoupled from the aerosol layer close to the surface, and the differences are around 17 % for both retrievals. In general, all the discrepancies found are within the uncertainly limits, showing the robustness and reliability of the GRASP algorithm. However, the better agreement found for the Cerro Poyos retrieval with the aircraft data and the vertical homogeneity of certain properties retrieved with GRASP, such as the scattering Ångström exponent, for cases with aerosol layers characterized by different aerosol types, shows that uncertainties in the vertical distribution of the aerosol properties have to be considered. The comparison presented here between GRASP and other algorithms (i.e. AERONET and LIRIC) and with airborne in situ measurements shows the potential to retrieve the optical and microphysical profiles of the atmospheric aerosol properties. Also, the advantage of GRASP versus LIRIC is that GRASP does not assume the results of the AERONET inversion as a starting point. 1 Introduction Atmospheric aerosols play an important role in the Earth– atmosphere radiative system due to their interaction with so- Published by Copernicus Publications on behalf of the European Geosciences Union.
4440 J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada lar and terrestrial radiation and their role in cloud development and precipitation (Boucher et al., 2013). Uncertainties associated with the interaction of atmospheric aerosols with radiation have been reduced in the last years, but there is still a need for improvement, mainly in those aspects related to their absorption properties (IPCC, 2013). The characterization of aerosol vertical distribution is another point of interest to reduce uncertainties associated with atmospheric aerosol particles, since they can be different near the surface, within the boundary layer and in the free troposphere. Passive remote sensing offers large advances in aerosol characterization with global sun-photometry networks such as the Aerosol Robotic Network (AERONET; Holben et al., 1998) or lunar and/or star photometry measurements (Pérez- Ramírez et al., 2012; Barreto et al., 2016, 2017). In the last few years, several different inversion methods, based on spectral aerosol optical depth (AOD) measurements, were developed for the retrieval of aerosol microphysical properties such as effective radius (reff) and volume concentration (VC) (e.g. Pérez-Ramírez et al., 2015; Torres et al., 2017). Furthermore, other sophisticated algorithms that use sky radiance measurements were developed for the retrieval of aerosol microphysical properties as well as intensive properties such as single-scattering albedo (SSA), asymmetry parameter and aerosol refractive index (RI) (e.g. Nakajima et al., 1996; Dubovik and King, 2000; Olmo et al., 2006, 2008). Nevertheless, all these algorithms and measurements only provide column-integrated aerosol properties. Since the 1970s, lidar systems have been widely used to characterize aerosol vertical distributions in order to contribute to reducing the radiative forcing uncertainties associated with the atmospheric aerosol. The most basic systems use only information about the elastic lidar signal to derive backscatter coefficient by aerosol particles but require an assumption about the extinction-to-backscatter ratio (lidar ratio, LR) (Fernald et al., 1972; Klett, 1981, 1985; Fernald, 1984). More advanced systems such as Raman (Ansmann et al., 1992; Whiteman et al., 1992) and HSRL (High Spectral Resolution Lidar) (Shipley et al., 1983; Grund and Eloranta, 1991) are able to provide independent measurements of backscatter and extinction coefficients (βand α, respectively) without LR assumption. Also, the depolarization measurements are a lidar improvement that provide information about the shape of aerosols and allow us to characterize the aerosol type (Murayama et al., 2004; Miffre et al., 2011; Bravo-Aranda et al., 2013). However, lidar observations dedicated to the aerosol characterization are very scarce compared to the sun-photometer measurements, and many international networks have emerged in the last decades to homogenize and explore such information. This is the case of the global NASA MPLNET network (Micro-Pulse Lidar Network; Lewis et al., 2016) developed for continuous measurements of aerosol and cloud vertical profiles at different sites in the world using standard instrument and data processing algorithms. The EARLINET (European Aerosol Research LIdar NETwork; Pappalardo et al., 2014) and LALINET (Latin American LIdar NETwork; Guerrero-Rascado et al., 2016) have also been established in order to provide long-term database for the vertical and temporal distribution of aerosols over Europe and Latin America, respectively. The retrieval of particle vertical microphysical properties from multiwavelength lidar systems is possible by inverting measurements of three aerosol backscatter and two extinction coefficients, known as the 3β+2αconfiguration, using the algorithms developed by Müller et al. (1999), Böckmann (2001) and Veselovskii et al. (2002). However, 3β+2αmeasurements are scarce compared with the large database of elastic lidar measurements. In this sense, different inversion methods were recently developed within the framework of EARLINET in order to retrieve vertical profiles of aerosol microphysical properties using combined information of elastic lidar and sun-photometry measurements. These approaches were the LIdar-Radiometer Inversion Code (LIRIC; Chaikovsky et al., 2008, 2012, 2016), which provides vertical distribution of volume concentrations, and the Generalized Aerosol Retrieval from Radiometer and Lidar Combined data (GARRLiC; Lopatin et al., 2013), which also allows the retrieval of SSA and RI. Currently, GARRLiC algorithm is included in the Generalized Retrieval of Atmosphere and Surface Properties inversion code (GRASP; Dubovik et al., 2011). However, very few studies have attempted to evaluate this recently developed inversion algorithm (Lopatin et al., 2013; Bovchaliuk et al., 2016; Torres et al., 2017; Román et al., 2017), and therefore their evaluation under different atmospheric conditions is still necessary. Field campaigns with state-of-the-art instrumentation offer unique possibilities for the evaluation of new retrievals techniques of particle microphysical and optical properties. Recently, the ADRIMED (Aerosol Direct Radiative Impact on the regional climate in the MEDiterranean region) field campaign, which was part of the international cooperative research program Chemistry-Aerosol Mediterranean Experiment (ChArMEx; Dulac, 2014), was carried out with the main objective of capturing the high complexity of the different aerosol types in the Mediterranean region (Mallet et al., 2016). Several in situ and remote sensing measurements both from surface and on airborne platforms were collected during this campaign using state-of-the-art instrumentation. The measurements were performed at different stations over the western Mediterranean region during summer 2013 to create an updated database of the physical, chemical and optical aerosol properties as well as the vertical distribution of the major “Mediterranean aerosols” (Mallet et al., 2016; Denjean et al., 2016). Data gathered during ChArMEx-ADRIMED campaign give us an excellent opportunity to evaluate the recently developed algorithms for retrieving aerosol microphysical and optical profiles. In that framework, the main objective of this study is to evaluate the aerosol optical and microphysical proper- Atmos. Meas. Tech., 10, 4439–4457, 2017 www.atmos-meas-tech.net/10/4439/2017/
J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada 4441 ties obtained with GRASP during the ChArMEx-ADRIMED field campaign in Granada, Spain. The GRASP configuration evaluated in this study here is the one that combines lidar signals and sun–sky radiance measurements. The paper is structured as follows: Sect. 2 gives a brief description of the experimental site and the instrumentation employed in this study. GRASP and LIRIC codes are described in detail in Sect. 3. The results are discussed in Sect. 4 and, finally, the main conclusions are summarized in Sect. 5. 2 Site and instrumentation 2.1 Experimental site The experimental measurements were obtained over Granada (Spain) at the Andalusian Institute for Earth System Research (IISTA-CEAMA) of the University of Granada, Spain (37.16◦N, 3.61◦W; 680 ma.s.l.), and at the remote high mountain site Cerro Poyos (37.11◦N, 3.49◦W; 1820ma.s.l.) located at the Sierra Nevada mountain range, about 12km away (horizontally) from IISTA-CEAMA station. Figure 1 shows a map illustrating the distance between the Granada and Cerro Poyos stations. The city of Granada is located in south-eastern Iberian Peninsula and is a non-industrialized medium-sized city with a population around 300000 (twice including the metropolitan area). The city is sited in a natural basin surrounded by mountains with elevations between 1000 and 3500ma.s.l. The area is approximately 200 km from the African continent and approximately 50km from the western Mediterranean basin. In Granada, one main source of natural aerosol is the long-range transport of mineral dust particles from North Africa (e.g. Lyamani et al., 2005; Valenzuela et al., 2012a) that reaches the area in lofted layers (Müller et al., 2009; Guerrero-Rascado et al., 2008, 2009; Córdoba-Jabonero et al., 2011) before mixing with the atmospheric boundary layer (Bravo-Aranda et al., 2015) and been detected at the surface in precipitation samples (Calvo et al., 2010). Another natural source is biomass burning particles: fresh smoke (Alados-Arboledas et al., 2011) and longrange transported smoke (Ortiz-Amezcua et. al., 2014, 2017). While the main anthropogenic sources are pollution from Europe, the Iberian Peninsula and the Mediterranean Sea (Lyamani et al., 2006; Pérez-Ramírez et al., 2016), local sources are mainly road traffic and central heating systems (Lyamani et al., 2012; Titos et al., 2017). 2.2 Ground-based instrumentation Columnar aerosol properties during daytime were obtained by CIMEL CE-318-4 (Cimel Electronique) sun–sky photometers at IISTA-CEAMA and Cerro Poyos sites. The sunphotometer instruments used in this study are operated in the framework of AERONET-RIMA network (Iberian Network for Aerosol Measurements, infrastructure of AERONET) (https://aeronet.gsfc.nasa.gov/). A complete description of Figure 1. Map illustrating the Granada and Cerro Poyos stations. The red line indicates the trajectory and the black points show the altitude of the aircraft on 17 June. the instrument can be found in Holben et al. (1998). Briefly, this instrument makes direct solar irradiance measurements at 340, 380, 440, 670, 870 and 1020nm and sky radiance measurements at 440, 670, 870 and 1020nm. Solar direct irradiance measurements are used to calculate the AOD at 340, 380, 440, 670, 870 and 1020nm, with uncertainty of ±0.01 for λ > 400nm and of ±0.02 for λ < 400nm (Holben et al., 1998; Eck et al., 1999). Furthermore, the Ångström exponent (AE), a parameter that describes the spectral dependency of the AOD, is calculated in the range of 440–870nm. The AE provides an indication of the particle size: small values (<0.5) suggest a predominance of coarse particles, while large values (>1.5) indicate a predominance of small particles (e.g. Dubovik et al., 2002). The solar direct irradiance and sky radiance measurements are used to retrieve aerosol optical and microphysical properties such as columnar particle size distribution (PSD), real and imaginary refractive indices (RRI and IRI) and SSA, using the algorithm of Dubovik et al. (2006). In addition, the inversion code provides other variables such as the VC, reff and standard deviation for fine and coarse modes of the retrieved PSD. The uncertainty of the AERONET inversion products is described by Dubovik et al. (2000). Briefly, the uncertainty in the retrieval of SSA is ±0.03 for high aerosol load (AOD440 >0.4) and solar zenith angle >50◦. For measurements with low aerosol load (AOD440 <0.2), the retrieval accuracy of SSA (λ) drops down to 0.02–0.07 (Dubovik et al., 2000). For high aerosol load and solar zenith angle>50◦, errors are about 30–50% for the imaginary part of the RI. For particles in the size range 0.1< r < 7 µm, errors in PSD retrievals are around 10–35%, while for sizes lower than 1 µm and higher than 7 µm retrieval errors rise up to 80–100%. In this work, the AERONET Version 2 Level 2.0 data obtained at Granada and Cerro Poyos during www.atmos-meas-tech.net/10/4439/2017/ Atmos. Meas. Tech., 10, 4439–4457, 2017
4442 J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada Table 1. Instruments on board the ATR-42 aircraft during F30 and F31 flights. Parameter Instrument Abbreviation Scientific objective Nominal size Wavelength measured range (µm) (nm) Size distribution Forward scattering spectrometer FSSP-300 Coarse mode concentration 0.28–20 632.8probe, model 300, Particle Measuring Systems Sky optical particle counter, GRIMM Coarse mode concentration 0.25–32 655 model 1.129, Grimm Technik Ultra high-sensitivity aerosol UHSAS Aiken+accumulation 0.04–1 1054spectrometer, Droplet mode concentration Measurement Technologies Scanning mobility particle sizer, SMPS Aiken+accumulation 0.03–0.4 n/a∗ custom-built mode concentration Optical properties 3λintegrated nephelometer, Nephelometer Scattering coefficient n/a∗450, 550, 700 model 3563, TSI Cavity attenuated phase shift, CAPS Extinction coefficient n/a∗530 Aerodyne Research Inc. Photomètre Léger Aéroporté pour PLASMA Extinction coefficient, n/a∗340–2250 la Surveillance des Masses d’Air AOD ∗Not applicable. ChArMEx-ADRIMED 2013 are used. However, due to the strong limitations imposed by the AERONET inversion algorithm (AOD440 >0.4 and solar zenith angle >50◦), there was no SSA and RI AERONET Level 2.0 retrievals during the campaign. Thus, for comparing AERONET SSA values with GRASP retrievals, the AERONET Level 1.5 cloud screened data corresponding to AOD >0.2 and solar zenith angle>50◦are used in this study. The multiwavelength Raman lidar MULHACEN, based on a customized version of LR331D400 (Raymetrics S.A.), is used for obtaining vertical profiles of the atmospheric aerosol properties. This system, located at Granada, was incorporated to EARLINET in April 2005 and at present a contributing station to ACTRIS research infrastructure (Aerosols, Clouds, and Trace gases Research InfraStructure Network; http://actris2.nilu.no/). The system has a monostatic biaxial configuration alignment, pointing vertically to the zenith and uses a pulsed Nd:YAG laser with second- and third-harmonic generators, that emits simultaneously pulses at 1064, 532 and 355nm. The receiving system consists of several detectors, which can split the radiation according to the three elastic channels at 355, 532 (parallel- and perpendicular-polarized; Bravo-Aranda et al., 2013) and 1064nm; two nitrogen Raman channels at 387 and 607 nm (shifted signal from radiation at 355 and 532nm, respectively); and a water vapour Raman channel at 408 nm (shifted signal from radiation at 355nm; Navas-Guzmán et al., 2014). More information can be found in Guerrero-Rascado et al. (2008). The aerosol particle backscatter coefficient profiles obtained from the multiwavelength lidar were obtained by the Klett–Fernald method (Fernald et al., 1972; Fernald, 1984; Klett, 1981, 1985). Total uncertainty in the profiles obtained with Klett method is usually 20% for βand 25–30% for αprofiles (Franke et al., 2001; Preißler et al., 2011). The procedure suggested by Wandinger and Ansmann (2002) was applied to the lidar data to correct the incomplete overlap. Without correction, the complete overlap for this instrument is above 1200 m a.g.l. (Navas-Guzmán et al., 2011). 2.3 Airborne measurements During the period from 14 June to 4 July 2013, 16 flights were performed in the framework of ChArMEx-ADRIMED over the Mediterranean Basin with the ATR-42 aircraft of SAFIRE (French aircraft service for environmental research; http://www.safire.fr). These flights ascended or descended performing a spiral trajectory during 30 min. Two of these flights (flight number F30 and F31) took place over Granada on 16 and 17 June 2013, respectively. Figure 1 shows the spiral trajectory of F31 flight that is similar to that of F30, covering in both cases the same atmospheric column. Flight details are described by Mallet et al. (2016) and Denjean et al. (2016). Table 1 summarizes the instrumentation on board the ATR-42 airplane used in this study. The scanning mobility particle sizer (SMPS) with an accuracy of 5% (Wiedensohler et al., 2012) and the ultra high-sensitivity aerosol spectrometer (UHSAS) with an accuracy of 10% (Cai et al., 2008) are used for measuring aerosol number size distribution in Atmos. Meas. Tech., 10, 4439–4457, 2017 www.atmos-meas-tech.net/10/4439/2017/
J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada 4443 Table 2. Input and output information used for LIRIC and GRASP retrievals. LIRIC GRASP Input Sun Lidar Sun Lidar photometer∗Elastic backscattered photometer Elastic backscattered – AOD signal: – AOT or AOD signal: – VC – 355, 532 and 1064nm – Total scattered – 355, 532 and – RRI and IRI – 532 cross-polarized radiances 1064nm – % sphericity signal At 440, 670, 870 and 1020nm Output – VC profile for fine and coarse mode Columnar (fine and coarse) Vertical (fine and coarse) – PSD – VC – RRI and IRI – αand β – VC – SSA –reff – SSA – LR – % sphericity (total) ∗AERONET product. the submicron range. The wing-mounted Forward Scattering Spectrometer Probe (FSSP-300) with an accuracy of 30% (Baumgardner et al., 1992) and the in-cabin GRIMM OPC (sky OPC 1.129) with an accuracy of 10 % (Denjean et al., 2016) were used to measure the optical size distributions in the diameter nominal size range between 0.28 and 20µm and between 0.3 and 32µm, respectively. The total particle volume concentrations in the diameter range 0.1–30µm and volume concentrations of fine (0.1–1µm) and coarse (1–30µm) modes were calculated from the measured aerosol number size distributions, assuming that aerosol particles are spherical. In addition, the nephelometer TSI (model 3563) was used to measure particle scattering coefficients at three wavelengths (450, 550 and 700nm) with an accuracy of 5% (Müller et al., 2011) and a cavity attenuated phase shift (CAPS) was employed to obtain particle extinction coefficient at 530 nm with an accuracy of 3% (Massoli et al., 2010). Also, the PLASMA (Photomètre Léger Aéroporté pour la Surveillance des Masses d’Air) system, which is an airborne sun-tracking photometer, was used to obtain AOD with wide spectral coverage (15 channels between 0.34 and 2.25µm) with an accuracy of approximately 0.01 (Karol et al., 2013), as well as the particle extinction vertical profiles (Torres et al., 2017). 3 GRASP and LIRIC inversion algorithms The input information needed by the GRASP and LIRIC algorithms and the aerosol properties retrieved and used in this work are shown in Table 2. The LIRIC algorithm provides height-resolved aerosol VC data for the fine and coarse modes from combined lidar and sun–sky photometer information (Chaikovsky et al., 2008, 2012, 2016; Granados- Muñoz et al., 2014). For this, column-integrated aerosol properties provided by the AERONET code (Dubovik et al., 2002, 2006) are used as input, together with the lidar elastic backscatter signals at three different wavelengths (355, 532, and 1064nm). These data are put through an iterative procedure based on the Levenberg–Marquardt method, which is described in detail in Chaikovsky et al. (2016). Besides the VC, the algorithm retrieves additional datasets, including profiles of particle αand βcoefficients, and LR, among others. AERONET column-integrated products used as input are not modified by LIRIC during the retrieval process. The GRASP inversion code (Dubovik et al., 2011; Lopatin et al., 2013) was developed at Laboratoire d’Optique Atmospherique (LOA) of the University of Lille. GRASP is based on a similar philosophy than LIRIC code but goes a step further since it simultaneously inverts both the coincident lidar and sun–sky photometer measurement, retrieving vertical, but also column, aerosol optical and microphysical properties for both fine and coarse modes. The simultaneous inversion of lidar and sun–sky photometer measurements is expected to improve the retrievals since the lidar data complement the sky photometer measurement at scattering angles of 180◦and the photometer data provide the information (e.g. amount and type) required for lidar retrievals that otherwise would be assumed from climatological data (Bovchaliuk et al., 2016). Therefore, the column aerosol properties obtained by GRASP will differ from the AERONET ones. Additionally, it is worth to note that GRASP allows independently retrieving aerosol optical and microphysical properties for the two distinct aerosol modes, fine and coarse. The retrieval of height-dependent SSA data is an additional advantage of GRASP over LIRIC. GRASP also provides an estimation of the systematic and random errors for both the directly retrieved (PSD, RRI, IRI, SSA) and derived (α,β, www.atmos-meas-tech.net/10/4439/2017/ Atmos. Meas. Tech., 10, 4439–4457, 2017
4444 J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada Figure 2. Temporal evolution of the lidar range-corrected signal (a, b) and the depolarization ratio (c, d) at 532 nm on 16 (a, c) and 17 (b, d) June 2013. The two purple lines indicate the lidar analysed interval. The black dashed line indicates the sun-photometer measurements. VC profiles) aerosol properties. The SSA profiles errors are not shown because they are unfortunately not provided at the moment. Additional details on GRASP retrieval algorithm and its performance can be found in Lopatin et al. (2013) and Bovchaliuk et al. (2016). 4 Results As previously mentioned, two of the ATR-42 flights performed in the framework of ChArMEx-ADRIMED campaign, F30 and F31, were carried out over Granada on 16 and 17 June 2013, respectively. Figure 2 shows the time series of the lidar range-corrected signal (RCS) and the depolarization ratio (δ) at 532nm on both days measured at Granada station. The RCS is calculated as P·r2, where Pis the lidar signal (corrected from background and dark current) and ris the altitude. On the first day, a homogeneous layer is observed from the surface up to 5km a.s.l., with an elevated aerosol layer coupled to the superficial aerosol layer throughout the day. The next day this layer was decoupled from the aerosol layer close to surface and disappeared around 13:00UTC; measurements of δshowed that there was an aerosol type below 2.7 km a.s.l. and another aerosol type above this altitude, up to 5.5kma.s.l. On 16 June, the lidar measurements (marked with purple lines in Fig. 2) obtained during the first flight between 14:15 and 14:45UTC and sun-photometer measurements collected at 16:22UTC (black dashed line in Fig. 2) at Granada and Cerro Poyos were selected for further analysis. The selected sun-photometer measurement was the closest measurement available in time to the first flight. On 17 June, the lidar measurements obtained during the second flight (07:15 to 07:45UTC) and sun–sky photometer measurements obtained at both stations at 07:40UTC were selected for further analysis. AERONET products during these flights indicate the presence of dust particles. In fact, on 16 June AOD440 at 14:15UTC was around 0.26 and 0.19 for Granada and Cerro Poyos, respectively, and 0.27 and 0.22 at 16:22UTC. On this day, the AE440−870 was 0.30–0.26 (Granada–Cerro Poyos) at 14:30UTC and 0.34–0.27 (Granada–Cerro Poyos) at 16:22UTC, indicating moderate atmospheric aerosol load dominated by coarse particles. On 17 June, the AOD440 at 07:40UTC was 0.21 and 0.18 and the AE440−870 was 0.43 and 0.30 for Granada and Cerro Poyos, respectively, which also indicates the predominance of coarse particles on this day. The presence of mineral dust over Granada during both days is confirmed by the analysis of back-trajectory analysis (not shown) by HYSPLIT (Hybrid Single-Particle Lagrangian Integrated Trajectory; Stein et al., 2015; Rolph, 2016), which indicates that the relevant air masses came from the Saharan region, specifically from Algeria, at different heights. 4.1 Comparison of columnar properties retrieved by GRASP and AERONET algorithms Some of the aerosol columnar properties obtained from AERONET and retrieved by GRASP (combining photometer and lidar measurements) on 16 and 17 June at Granada and Cerro Poyos stations are shown in Figs. 3–5 and summarized in Table 3. Figure 3 shows the column-integrated PSD retrieved by both AERONET and GRASP algorithms on 16 and 17 June for Granada and Cerro Poyos stations. The retrieved PSD evidence the predominance of coarse mode particles, as expected for dust events (Lyamani et al., 2005; Guerrero- Atmos. Meas. Tech., 10, 4439–4457, 2017 www.atmos-meas-tech.net/10/4439/2017/
J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada 4445 Table 3. Columnar effective radius and particle volume concentration for coarse and fine particle modes retrieved by GRASP and AERONET algorithms. 16 June 2013 17 June 2013 Granada Cerro Granada Cerro Poyos Poyos Effective GRASP fine 0.12 0.13 0.10 0.12 radius coarse 2.2 2.2 2.4 2.2 (µm) AERONET fine 0.12 0.11 0.11 0.12 coarse 1.9 1.9 2.1 1.9 Volume GRASP fine 0.018 0.017 0.018 0.011 concentration coarse 0.17 0.15 0.14 0.13 (µm3µm−2) AERONET fine 0.015 0.015 0.016 0.010 coarse 0.14 0.13 0.12 0.11 Figure 3. Size distribution retrieved by GRASP (blue) with its uncertainty (shaded area) and by AERONET (green) on 16 (a, b) and 17 (c, d) June 2013 at Granada (a, c) and Cerro Poyos (b, d). Rascado et al, 2009). Both AERONET and GRASP retrieved PSD present a bimodal behaviour, with the radius of fine mode below 0.5 µm and the radius of coarse mode above 0.5 µm. The differences between the PSD retrieved by GRASP and AERONET are mostly within uncertainties associated with both methods (±10–35% for the size range from 0.1 to 7µm and ±35–100% outside this range; Dubovik et al., 2000) except for the size range 5–8.7µm, where the differences are higher, especially at 6.64µm (>100 %). Furthermore, the coarse mode retrieved by GRASP over both sites shows a clear shift towards higher radii in comparison to the AERONET retrievals (Fig. 3). This shift was also observed by Lopatin et al. (2013) during dust and biomass burning events over Minsk, Belarus, and by Bovchaliuk et al. (2016) during dust events over Dakar, Senegal. These authors attributed this coarse mode shift towards higher radii to the use of the lidar data in the GRASP retrievals. The lidar data provide additional information at scattering angles of 180◦and further wavelengths compared to the sun photometer, influencing the size distribution retrieved especially in the coarse mode. Table 3 summarizes the columnar reff and VC of fine and coarse modes obtained at both stations by AERONET and GRASP algorithms on 16 and 17 June. The retrieved miwww.atmos-meas-tech.net/10/4439/2017/ Atmos. Meas. Tech., 10, 4439–4457, 2017
4446 J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada Figure 4. Spectral real (RRI) and imaginary (IRI) refractive indices retrieved by GRASP for the fine (blue) and coarse (red) modes with its uncertainty (shaded area), by AERONET (green) and by airborne measurement (black) on 16 (a, b) and 17 (c, d) June 2013 in Granada (a, c) and Cerro Poyos (b, d). crophysical properties are similar to those typically obtained during African desert dust events over Granada (Valenzuela et al., 2012b). The fine mode reff retrieved by both methods ranges between 0.10 and 0.13µm. Differences between fine mode reff retrieved by GRASP and AERONET are below 0.02 µm, which are within the uncertainty of the inversions (Lopatin et al., 2013; Torres et al., 2014). For the coarse mode, the reff values obtained by GRASP were 0.03 µm higher than those retrieved by AERONET but the differences are within the uncertainty range. A similar behaviour is observed for the column-integrated VC, with slightly larger values provided by GRASP for the fine and coarse modes (0.016±0.003 and 0.148 ±0.017 µm3µm−2) compared to AERONET (0.014±0.003 and 0.125±0.013 µm3µm−2), but differences are still within the uncertainties. Figure 4 illustrates the retrieved columnar RRI and IRI for each day obtained by GRASP and AERONET at Granada and Cerro Poyos. Moreover, RRI and IRI at 530 nm estimated by Denjean et al. (2016) using airborne measurements over Granada on 16 and 17 June are included in the plot. AERONET provides RRI and IRI for the whole size distribution, while GRASP is able to provide RRI and IRI for fine and coarse modes separately. The RRI retrieved by GRASP and AERONET algorithms do not show any spectral wavelength variations, and the differences between RRI values retrieved by both inversion algorithms are within the uncertainties (differences below 5%). Because of the predominance of the coarse mode during the analysed dust event, both the AERONET and airborne RRI values are close to the values retrieved by GRASP for the coarse mode, with differences <0.03, on both days. In contrast, the IRI values retrieved by GRASP for the fine mode present a rather low spectral dependence while IRI values for the coarse mode presents a clear increase in the UV region. These results are coherent with those reported for different absorption species by Schuster et al. (2016) using AERONET data. At Cerro Poyos we did not find the spectral dependence of the IRI typically associated with mineral dust. The AOD at 440nm was around 0.18–0.27 and we used AERONET Level 1.5 products; therefore, these values have large uncertainties (>50%; Dubovik et al., 2000). The lack of spectral dependence can be just an artifact of the inversion. However, it is worthy to note that at Cerro Poyos the PSD shows a mode in the coarse mode size range around 1µm. As there is still discussion in the scientific community about dust RI and about the differences in dust particles between different sources (e.g. Colarco et al., 2014), results can suggest possible differences in dust RI between long-range transported and mixture Atmos. Meas. Tech., 10, 4439–4457, 2017 www.atmos-meas-tech.net/10/4439/2017/
J. A. Benavent-Oltra et al.: Comparative assessment of GRASP algorithm for a dust event over Granada 4447 Figure 5. Single-scattering albedo retrieved by GRASP (blue) with its uncertainty (shaded area), by AERONET (green) and by airborne measurement (black) with its uncertainty on 16 (a, b) and 17 (c, d) June 2013 at Granada (a, c) and Cerro Poyos (b, d). with local dust injections (the area is very dry in summer, thus favouring local mineral dust resuspension) and local pollution. The RRI and IRI values provided by AERONET show good agreement with GRASP retrievals for the coarse mode, something expected due to the large predominance of dust particles. Better agreement between IRI retrieved by AERONET and by GRASP for the coarse mode was found for Cerro Poyos, with differences ∼10 %, while for Granada these differences are between 35 and 80% (larger differences at lower wavelengths). The high discrepancy between IRI retrieved by AERONET and by GRASP in the case of Granada can be explained by the uncertainty associated with the incomplete lidar overlap. Cerro Poyos station is located above the lidar incomplete overlap height, and thus the effect of the incomplete overlap on the retrieval is negligible. This is not the case for the retrieval from Granada station. On 16 June, IRI airborne values estimated at 530 nm are close to IRI retrieved by GRASP at 532nm for the coarse mode, and the differences are within the associated uncertainties. In contrast, on 17 June, there are more differences between IRI values retrieved by GRASP at Granada station and those estimated from airborne measurement, with differences over 100%, whereas for the Cerro Poyos retrievals the differences are 50%. Figure 5 shows the columnar SSA values retrieved by GRASP and AERONET on 16 and 17 June at Granada and Cerro Poyos. Moreover, the SSA value at 530 nm calculated by Denjean et al. (2016) for dust layers using airborne measurements during the campaign was 0.95±0.04. SSAs retrieved by GRASP at 532nm are close to the airborne value. Better agreement with this value is found for the retrievals from Granada on 16 June and at Cerro Poyos on 17 June. The differences from Granada on 17 June could be due to the fact that the in situ value was calculated for the dust layer whereas GRASP and AERONET use sun-photometer data, which measure the total atmospheric column. Furthermore, in the case of Granada station, these measurements could be influenced by injections of local pollution. The retrieved SSA values are in the range of 0.85–0.98 (355–1064 nm wavelength range), the typical values for dust aerosols (Dubovik et al., 2002; Toledano et al., 2011; Lopatin et al., 2013). Both AERONET and GRASP retrievals follow the same pattern with wavelength, with increasing SSA as wavelength increases, which is a typical characteristic of dust aerosols (Dubovik et al., 2002; Valenzuela et al., 2012b). Differences between SSA retrieved by AERONET and GRASP algorithms are below 0.03 at all wavelengths, within the uncertainties associated with each method. The discrepancies between SSA retrieved by AERONET and GRASP algorithms are obtained for Cerro Poyos station (<1%) at 1020 nm in particular, whereas for Granada retrievals the differences are bigger and the lowest discrepancies are obtained at 675 nm. www.atmos-meas-tech.net/10/4439/2017/ Atmos. Meas. Tech., 10, 4439–4457, 2017
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