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Comparison of Dust Optical Depth From Multi-Sensor Products and MONARCH (Multiscale Online Non-hydrostatic AtmospheRe CHemistry) Dust Reanalysis Over North Africa, the Middle East, and EuropeAerosol reanalysis datasets are model-based, observationally constrained, continuous 3D aerosol fields with a relatively high temporal frequency that can be used to assess aerosol variations and trends, climate effects, and impacts on socioeconomic sectors, such as health. Here we compare and assess the recently published MONARCH (Multiscale Online Non-hydrostatic AtmospheRe CHemistry) high-resolution regional desert dust reanalysis over northern Africa, the Middle East, and Europe (NAMEE) with a combination of ground-based observations and space-based dust retrievals and products. In particular, we compare the total and coarse dust optical depth (DOD) from the new reanalysis with DOD products derived from MODIS (MODerate resolution Imaging Spectroradiometer), MISR (Multi-angle Imaging SpectroRadiometer), and IASI (Infrared Atmospheric Sounding Interferometer) spaceborne instruments. Despite the larger uncertainties, satellite-based datasets provide a better geographical coverage than ground-based observations, and the use of different retrievals and products allows at least partially overcoming some single-product weaknesses in the comparison. Nevertheless, limitations and uncertainties due to the type of sensor, its operating principle, its sensitivity, its temporal and spatial resolution, and the methodology for retrieving or further deriving dust products are factors that bias the reanalysis assessment. We, therefore, also use ground-based DOD observations provided by 238 stations of the AERONET (AErosol RObotic NETwork) located within the NAMEE region as a reference evaluation dataset. In particular, prior to the reanalysis assessment, the satellite datasets were evaluated against AERONET, showing moderate underestimations in the vicinities of dust sources and downwind regions, whereas small or significant overestimations, depending on the dataset, can be found in the remote regions. Taking these results into consideration, the MONARCH reanalysis assessment shows that total and coarse-DOD simulations are consistent with satellite- and ground-based data, qualitatively capturing the major dust sources in the area in addition to the dust transport patterns. Moreover, the MONARCH reanalysis reproduces the seasonal dust cycle, identifying the increased dust activity that occurred in the NAMEE region during spring and summer. The quantitative comparison between the MONARCH reanalysis DOD and satellite multi-sensor products shows that the reanalysis tends to slightly overestimate the desert dust that is emitted from the source regions and underestimate the transported dust over the outflow regions, implying that the model's removal of dust particles from the atmosphere, through deposition processes, is too effective. More specifically, small positive biases are found over the Sahara desert (0.04) and negative biases over the Atlantic Ocean and the Arabian Sea (−0.04), which constitute the main pathways of the long-range dust transport. Considering the DOD values recorded on average there, such discrepancies can be considered low, as the low relative bias in the Sahara desert (< 50 %) and over the adjacent maritime regions (< 100 %) certifies. Similarly, over areas with intense dust activity, the linear correlation coefficient between the MONARCH reanalysis simulations and the ensemble of the satellite products is significantly high for both total and coarse DOD, reaching 0.8 over the Middle East, the Atlantic Ocean, and the Arabian Sea and exceeding it over the African continent. Moreover, the low relative biases and high correlations are associated with regions for which large numbers of observations are available, thus allowing for robust reanalysis assessment.
Document ID
20230009923
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Michail Mytilinaios ORCID
(Institute of Methodologies for Environmental Analysis Tito, Italy)
Sara Basart ORCID
(Barcelona Supercomputing Center Barcelona, Spain)
Sergio Ciamprone
(Institute of Methodologies for Environmental Analysis Tito, Italy)
Juan Cuesta ORCID
(Universités Paris-Est Créteil et Paris Créteil, France)
Claudio Dema
(Institute of Methodologies for Environmental Analysis Tito, Italy)
Enza Di Tomaso
(Barcelona Supercomputing Center Barcelona, Spain)
Paola Formenti ORCID
(Université Paris Cité Paris, France)
Antonis Gkikas ORCID
(National Observatory of Athens Athens, Attiki, Greece)
Oriol Jorba ORCID
(Barcelona Supercomputing Center Barcelona, Spain)
Ralph Kahn ORCID
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Carlos Pérez García‐Pando ORCID
(Barcelona Supercomputing Center Barcelona, Spain)
Serena Trippetta
(Institute of Methodologies for Environmental Analysis Tito, Italy)
Lucia Mona
(Institute of Methodologies for Environmental Analysis Tito, Italy)
Date Acquired
July 5, 2023
Publication Date
May 17, 2023
Publication Information
Publication: Atmospheric Chemistry and Physics
Publisher: European Geosciences Union
Volume: 23
Issue: 9
Issue Publication Date: May 1, 2023
ISSN: 1680-7316
e-ISSN: 1680-7324
URL: https://acp.copernicus.org/articles/23/5487/2023/
Subject Category
Geosciences (General)
Earth Resources and Remote Sensing
Funding Number(s)
WBS: 921266.04.12.01.64
CONTRACT_GRANT: EUH 2020 690462
CONTRACT_GRANT: EUH 2020 871115
CONTRACT_GRANT: Avviso MUR DD 2595 del 24.12.2019
CONTRACT_GRANT: EUH 2020 773051
CONTRACT_GRANT: EUH 2020 749461
CONTRACT_GRANT: AECT-2019-3-0001
CONTRACT_GRANT: AECT-2020-1-0007
CONTRACT_GRANT: AECT-2020-3-0013
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
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