4.5 Article

ModIs Dust AeroSol (MIDAS): a global fine-resolution dust optical depth data set

Journal

ATMOSPHERIC MEASUREMENT TECHNIQUES
Volume 14, Issue 1, Pages 309-334

Publisher

COPERNICUS GESELLSCHAFT MBH
DOI: 10.5194/amt-14-309-2021

Keywords

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Funding

  1. COST Action InDust [CA16202]
  2. COST (European Cooperation in Science and Technology)
  3. European Commission H2020 Marie Sklodowska-Curie Actions (DUST-GLASS) [749461]
  4. Marie Curie Actions (MSCA) [749461] Funding Source: Marie Curie Actions (MSCA)

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Monitoring and describing the spatiotemporal variability in dust aerosols is crucial for understanding their effects, feedbacks, and impacts within the Earth system. The MIDAS data set provides global daily dust optical depth data at fine spatial resolution over a 15-year period, combining satellite AOD retrievals with DOD-to-AOD ratios from reanalysis to derive DOD on the MODIS native grid. The uncertainties of the data set are taken into account for estimation of total DOD uncertainty, with good agreement and some deviations when compared to other monitoring sources.
Monitoring and describing the spatiotemporal variability in dust aerosols is crucial for understanding their multiple effects, related feedbacks, and impacts within the Earth system. This study describes the development of the ModIs Dust AeroSol (MIDAS) data set. MIDAS provides columnar daily dust optical depth (DOD) at 550 nm at a global scale and fine spatial resolution (0.1 degrees x 0.1 degrees) over a 15-year period (2003-2017). This new data set combines quality filtered satellite aerosol optical depth (AOD) retrievals from MODIS-Aqua at swath level (Collection 6.1; Level 2), along with DOD-to-AOD ratios provided by the Modern-Era Retrospective analysis for Research and Applications version 2 (MERRA-2) reanalysis to derive DOD on the MODIS native grid. The uncertainties of the MODIS AOD and MERRA-2 dust fraction, with respect to the AEronet RObotic NETwork (AERONET) and Lldar climatology of vertical Aerosol Structure for space-based lidar simulation (LIVAS), respectively, are taken into account for the estimation of the total DOD uncertainty. MERRA-2 dust fractions are in very good agreement with those of LIVAS across the dust belt in the tropical Atlantic Ocean and the Arabian Sea; the agreement degrades in North America and the Southern Hemisphere, where dust sources are smaller. MIDAS, MERRA-2, and LIVAS DODs strongly agree when it comes to annual and seasonal spatial patterns, with colocated global DOD averages of 0.033, 0.031, and 0.029, respectively; however, deviations in dust loading are evident and regionally dependent. Overall, MIDAS is well correlated with AERONET-derived DODs (R = 0.89) and only shows a small positive bias (0.004 or 2.7 %). Among the major dust areas of the planet, the highest R values (>0.9) are found at sites of North Africa, the Middle East, and Asia. MIDAS expands, complements, and upgrades the existing observational capabilities of dust aerosols, and it is suitable for dust climatological studies, model evaluation, and data assimilation.

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