Remote sensing of soot carbon – Part 2: Understanding the absorption Ångström exponent

dc.contributor.authorSchuster, G. L.
dc.contributor.authorDubovik, O.
dc.contributor.authorArola, A.
dc.contributor.authorEck, Thomas
dc.contributor.authorHolben, B. N.
dc.date.accessioned2024-02-15T22:43:17Z
dc.date.available2024-02-15T22:43:17Z
dc.date.issued2016-02-11
dc.description.abstractRecently, some authors have suggested that the absorption Ångström exponent (AAE) can be used to deduce the component aerosol absorption optical depths (AAODs) of carbonaceous aerosols in the AERONET database. This AAE approach presumes that AAE ≪ 1 for soot carbon, which contrasts the traditional small particle limit of AAE = 1 for soot carbon. Thus, we provide an overview of the AERONET retrieval, and we investigate how the microphysics of carbonaceous aerosols can be interpreted in the AERONET AAE product. We find that AAE ≪ 1 in the AERONET database requires large coarse mode fractions and/or imaginary refractive indices that increase with wavelength. Neither of these characteristics are consistent with the current definition of soot carbon, so we explore other possibilities for the cause of AAE ≪ 1. AAE is related to particle size, and coarse mode particles have a smaller AAE than fine mode particles for a given aerosol mixture of species. We also note that the mineral goethite has an imaginary refractive index that increases with wavelength, is very common in dust regions, and can easily contribute to AAE ≪ 1. We find that AAE ≪ 1 can not be caused by soot carbon, unless soot carbon has an imaginary refractive index that increases with wavelength throughout the visible and near-infrared spectrums. Finally, AAE is not a robust parameter for separating carbonaceous absorption from dust aerosol absorption in the AERONET database.
dc.description.sponsorshipThis material was supported by the National Aeronautics and Space Administration under the NASA Glory Science Team, issued through the Science Mission Directorate, Earth Science Division. Oleg Dubovik was supported by the Labex CaPPA project involving several research institutions in Nord-Pasde-Calais, France. Antti Arola acknowledges support from the Academy of Finland (through the project number 264242). We appreciate the efforts of the 29 AERONET and PHOTONS (Service d’Observation from LOA/USTL/CNRS) principal investigators and the entire AERONET and PHOTONS teams for obtaining, processing, documenting, and disseminating their respective data sets. Finally, we thank the anonymous reviewers for their time and effort.
dc.description.urihttps://acp.copernicus.org/articles/16/1587/2016/
dc.format.extent16 pages
dc.genrejournal articles
dc.identifierdoi:10.13016/m2scdc-pprq
dc.identifier.citationSchuster, G. L., Dubovik, O., Arola, A., Eck, T. F., and Holben, B. N.: Remote sensing of soot carbon – Part 2: Understanding the absorption Ångström exponent, Atmos. Chem. Phys., 16, 1587–1602, https://doi.org/10.5194/acp-16-1587-2016, 2016.
dc.identifier.urihttps://doi.org/10.5194/acp-16-1587-2016
dc.identifier.urihttp://hdl.handle.net/11603/31645
dc.language.isoen_US
dc.publisherEGU
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC GESTAR II Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rightsPublic Domain Mark 1.0 en
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titleRemote sensing of soot carbon – Part 2: Understanding the absorption Ångström exponent
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0001-9801-1610

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