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dc.contributor.authorGebhardt, C.
dc.contributor.authorAbuelgasim, A.
dc.contributor.authorFonseca, R. M.
dc.contributor.authorMartín-Torres, J.
dc.contributor.authorZorzano, M. P.
dc.date.accessioned2021-05-06T23:10:11Z
dc.date.available2021-05-06T23:10:11Z
dc.date.issued2021-03-16
dc.identifier.citationGebhardt , C , Abuelgasim , A , Fonseca , R M , Martín-Torres , J & Zorzano , M P 2021 , ' Characterizing Dust-Radiation Feedback and Refining the Horizontal Resolution of the MarsWRF Model Down to 0.5 Degree ' , Journal of Geophysical Research: Planets , vol. 126 , no. 3 , e2020JE006672 . https://doi.org/10.1029/2020JE006672en
dc.identifier.issn2169-9097
dc.identifier.otherPURE: 192769218
dc.identifier.otherPURE UUID: 0cd4d1b1-a0d4-4e31-acea-c2863d1a506b
dc.identifier.otherScopus: 85103561237
dc.identifier.otherORCID: /0000-0001-6479-2236/work/93483166
dc.identifier.urihttps://hdl.handle.net/2164/16406
dc.descriptionAcknowledgments Once again, our warmest thanks go to the PlanetWRF development team for providing the MarsWRF model free of charge to us and their proactive attitude in general. We would also like to thank two anonymous reviewers and the Associate Editor Dr Claire Newman for their several detailed and insightful comments and suggestions that helped to significantly improve the quality of the paper. We would like to acknowl- edge the support of this work by funding from the United Arab Emirates University (UAE University). Also, we are deeply grateful to High-Performance Computing, Division of Information Technology, UAE University, for the valuable access to the computational resources required for this work. We thank IT engineers Asma AlNeyadi, Anil Thomas, and Nithin Damodaran for their professional assistance and support in technical questions. M.-P. Z. has been partially funded by the AEI (MDM-2017-0737, Unity of Excellence “María de Maeztu” - Centro de Astro- biología (CSIC-INTA)) and the Spanish Ministry of Science and Innovation (PID2019-104205GB-C219). Finally, we declare that there are no real or perceived conflicts of interests for any author.en
dc.format.extent23
dc.language.isoeng
dc.relation.ispartofJournal of Geophysical Research: Planetsen
dc.rightsThis is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. https://creativecommons.org/licenses/by/4.0/en
dc.subjectdust cycleen
dc.subjectdust-radiation feedbacken
dc.subjectinteractive dusten
dc.subjectMarsWRF modelen
dc.subjectmodel resolutionen
dc.subjectprescribed dusten
dc.subjectQ Science (General)en
dc.subjectGeophysicsen
dc.subjectForestryen
dc.subjectOceanographyen
dc.subjectAquatic Scienceen
dc.subjectEcologyen
dc.subjectWater Science and Technologyen
dc.subjectSoil Scienceen
dc.subjectGeochemistry and Petrologyen
dc.subjectEarth-Surface Processesen
dc.subjectAtmospheric Scienceen
dc.subjectEarth and Planetary Sciences (miscellaneous)en
dc.subjectSpace and Planetary Scienceen
dc.subjectPalaeontologyen
dc.subjectOtheren
dc.subjectSupplementary Informationen
dc.subjecthttp://dx.doi.org/10.17632/ r7zm22h7x4.1en
dc.subject.lccQ1en
dc.titleCharacterizing Dust-Radiation Feedback and Refining the Horizontal Resolution of the MarsWRF Model Down to 0.5 Degreeen
dc.typeJournal articleen
dc.contributor.institutionUniversity of Aberdeen.Northern Rivers Institute (NRI)en
dc.contributor.institutionUniversity of Aberdeen.Planetary Sciencesen
dc.contributor.institutionUniversity of Aberdeen.Earth Systems and Environmental Sciencesen
dc.description.statusPeer revieweden
dc.description.versionPublisher PDFen
dc.identifier.doihttps://doi.org/10.1029/2020JE006672
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=85103561237&partnerID=8YFLogxKen


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