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dc.contributor.authorSurl, Luke
dc.contributor.authorPalmer, Paul I.
dc.contributor.authorAbad, Gonzalo González
dc.date.accessioned2021-12-21T14:53:01Z
dc.date.available2021-12-21T14:53:01Z
dc.date.issued2018-04-05
dc.identifier.citationSurl , L , Palmer , P I & Abad , G G 2018 , ' Which processes drive observed variations of HCHO columns over India? ' , Atmospheric Chemistry and Physics , vol. 18 , no. 7 , pp. 4549-4566 . https://doi.org/10.5194/acp-18-4549-2018en
dc.identifier.issn1680-7316
dc.identifier.otherPURE: 198030552
dc.identifier.otherPURE UUID: df1bb96e-1b9e-41f6-847f-bd020705b041
dc.identifier.otherORCID: /0000-0003-3085-2303/work/43322415
dc.identifier.otherScopus: 85045058080
dc.identifier.urihttps://hdl.handle.net/2164/17726
dc.descriptionLuke Surl was funded by the NERC National Centre for Earth Observation (NCEO020005), and Paul I. Palmer gratefully acknowledges his Royal Society Wolfson Research Merit Award. Luke Surl also acknowledges funding from the British Council Newton Fund (215829867), administered by the University of Birmingham. We are grateful to Kelly Chance from the Harvard-Smithsonian Center for Astrophysics, the Harvard University GEOS-Chem group, who maintains the model, and to Rolf Sander for maintaining the CAABA/MECCA box model.en
dc.format.extent18
dc.language.isoeng
dc.relation.ispartofAtmospheric Chemistry and Physicsen
dc.rightsThis work is distributed under the Creative Commons Attribution 4.0 License https://creativecommons.org/licenses/by/4.0/en
dc.subjectNatural Environment Research Council (NERC)en
dc.subjectThe British Councilen
dc.titleWhich processes drive observed variations of HCHO columns over India?en
dc.typeJournal articleen
dc.contributor.institutionUniversity of Aberdeen.Chemistryen
dc.description.statusPeer revieweden
dc.description.versionPublisher PDFen
dc.identifier.doihttps://doi.org/10.5194/acp-18-4549-2018
dc.identifier.urlhttps://doi.org/10.5194/acp-18-4549-2018en
dc.identifier.vol18en
dc.identifier.iss7en


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