Articles | Volume 18, issue 11
https://doi.org/10.5194/acp-18-8097-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/acp-18-8097-2018
© Author(s) 2018. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Insight into global trends in aerosol composition from 2005 to 2015 inferred from the OMI Ultraviolet Aerosol Index
Melanie S. Hammer
CORRESPONDING AUTHOR
Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
Randall V. Martin
Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
Chi Li
Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
Omar Torres
Atmospheric Chemistry and Dynamics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD, USA
Max Manning
Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
Brian L. Boys
Department of Physics and Atmospheric Science, Dalhousie University, Halifax, Nova Scotia, Canada
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Latest update: 14 Nov 2024
Short summary
We apply a simulation of the Ultraviolet Aerosol Index (UVAI), a method of detecting aerosol absorption from satellite observations, to interpret UVAI values observed by the Ozone Monitoring Instrument (OMI) from 2005 to 2015 to understand global trends in aerosol composition. We find that global trends in the UVAI are largely explained by trends in absorption by mineral dust, absorption by brown carbon, and scattering by secondary inorganic aerosol.
We apply a simulation of the Ultraviolet Aerosol Index (UVAI), a method of detecting aerosol...
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