High summertime aerosol loadings over the Arabian Sea and their transport pathways
Online Publication Date2018-09-24
Print Publication Date2018-09-27
Permanent link to this recordhttp://hdl.handle.net/10754/628708
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AbstractSatellite observations show high aerosol loadings over the Arabian Sea in boreal summer, which have great impacts on the Indian monsoon due to absorbing dust aerosols. However, the compositions, origins, transport pathways, and decadal trends of these aerosols have not been well studied. In this study, using multiple satellite retrievals, a back-trajectory model, and reanalysis data, we found that: 1) Aerosol optical depth (AOD) over the Arabian Sea and Arabian Peninsula have a summer peak and dust aerosols dominate the AOD; Aerosol reanalysis data tend to considerably underestimate dust AOD compared to satellite data, indicating challenges of extracting dust from total AOD; 2) Aerosols over the Arabian Sea are largely transported from South and East Arabian Peninsula by cyclonic winds in the lower troposphere (850 hPa) and from Iran–Afghanistan–Pakistan by anticyclonic winds in the middle troposphere (500 hPa); 3) Both case studies and composite analyses show that extremely high aerosol loadings over the Arabian Sea is associated with an abnormally low pressure over the Arabian Sea and the Middle East; and 4) Significant positive trends in AOD over the Arabian Peninsula and the Arabian Sea exist during 2000–2011 but disappear during 2000–2016, indicating a strong interdecadal variability of dust activities. This study revealed pathways linking dust emissions in the Middle East to high summertime AOD over the Arabian Sea and identified the atmospheric conditions favorable for dust emissions and transport.
CitationJin Q, Wei J, Pu B, Yang Z-L, Parajuli SP (2018) High summertime aerosol loadings over the Arabian Sea and their transport pathways. Journal of Geophysical Research: Atmospheres. Available: http://dx.doi.org/10.1029/2018jd028588.
SponsorsThe authors gratefully acknowledge the NOAA Air Resources Laboratory (ARL) for providing the HYSPLIT transport and dispersion model and the READY website (http://www.ready.noaa.gov) used in this publication. This work was supported by the Priority Academic Program Development of Jiangsu Higher Education Institutions (PAPD) and a start-up grant to J. Wei from the Nanjing University of Information Science and Technology.
PublisherAmerican Geophysical Union (AGU)