Spectral derivative analysis of solar spectroradiometric measurements: Theoretical basis

dc.contributor.authorHansell, R. A.
dc.contributor.authorTsay, S.-C.
dc.contributor.authorPantina, P.
dc.contributor.authorLewis, Jasper
dc.contributor.authorJi, Q.
dc.contributor.authorHerman, Jay
dc.date.accessioned2023-02-13T20:46:41Z
dc.date.available2023-02-13T20:46:41Z
dc.date.issued2014-06-21
dc.description.abstractSpectral derivative analysis, a commonly used tool in analytical spectroscopy, is described forstudying cirrus clouds and aerosols using hyperspectral, remote sensing data. The methodology employsspectral measurements from the 2006 Biomass-burning Aerosols in Southeast Asiafield study to demonstrate theapproach. Spectral peaks associated with thefirst two derivatives of measured/modeled transmitted spectralfluxes are examined in terms of their shapes, magnitudes,and positions from 350 to 750 nm, where variability islargest. Differences in spectral features between media aremainly associated with particle size and imaginary termof the complex refractive index. Differences in derivativespectra permit cirrus to be conservatively detected atoptical depths near the optical thin limit of ~0.03 and yield valuable insight into the composition and hygroscopicnature of aerosols. Biomass-burning smoke aerosols/cirrus generally exhibit positive/negative slopes, respectively,across the 500–700 nm spectral band. The effect of cirrus in combined media is to increase/decrease the slope ascloud optical thickness decreases/increases. For thick cirrus, the slope tends to 0. An algorithm is also presentedwhich employs a two modelfit of derivative spectra for determining relative contributions of aerosols/clouds tomeasured data, thus enabling the optical thickness of the media to be partitioned. For the cases examined,aerosols/clouds explain ~83%/17% of the spectral signatures, respectively, yielding a mean cirrus cloud opticalthickness of 0.08 ± 0.03, which compared reasonably wellwith those retrieved from a collocated Micropulse LidarNetwork Instrument (0.09 ± 0.04). This method permitsextracting the maximum informational content fromhyperspectral data for atmospheric remote sensing applications.en_US
dc.description.sponsorshipThis work is supported by the NASARadiation Sciences Program managedby Hal B. Maring. Both AERONET andMPLNET are funded by the NASA EarthObserving System and RadiationSciences Program. We would like tothank B. Holben for establishing andmaintaining the AERONET site at Phimaiand for the valuable discussions. Weacknowledge the MODTRAN developers(a joint collaboration of Spectral Sciences,Inc. and the U.S. Air Force) for their RTMcode and M. Hess for making the OPACdatabase publicly available. We wouldlike to thank G. Fager at PANalytical NIR(formerly ASD) for his technical supportof our FieldSpec Pro instrument andD. Feldman and T. O’Haven for theirMODTRAN wrapper and signal-processingcodes (terpconnect.umd.edu/~toh/spectrum/SignalProcessingTools.html),respectively. We also thank B. Baum,P. Yang, A. Heymsfield, and C. Schmitt fortheir ice cloud scattering models. Lastly,we thank the reviewers for their helpfuland insightful commentsen_US
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/full/10.1002/2013JD021423en_US
dc.format.extent17 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2d54i-u2lb
dc.identifier.citationHansell,R.A.,S.-C.Tsay,P.Pantina,J.R.Lewis,Q. Ji, and J. R. Herman (2014), Spectralderivative analysis of solar spectroradio-metric measurements: Theoretical basis,J. Geophys. Res. Atmos.,119,8908–8924. https://doi.org/10.1002/2013JD021423.en_US
dc.identifier.urihttps://doi.org/10.1002/2013JD021423
dc.identifier.urihttp://hdl.handle.net/11603/26812
dc.language.isoen_USen_US
dc.publisherAGUen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology
dc.relation.ispartofUMBC Faculty 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.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleSpectral derivative analysis of solar spectroradiometric measurements: Theoretical basisen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-9146-1632en_US
dcterms.creatorhttps://orcid.org/0000-0002-4263-9262en_US

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