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Automated width measurements of Martian dust devil tracks

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dc.contributor.authorStatella, Thiago
dc.contributor.authorPina, Pedro
dc.contributor.authorSilva, Erivaldo Antonio da [UNESP]
dc.contributor.institutionInst Fed Educ Ciencia & Tecnol Mato Grosso IFMT
dc.contributor.institutionUniv Lisbon
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2018-11-27T10:46:41Z
dc.date.available2018-11-27T10:46:41Z
dc.date.issued2016-03-01
dc.description.abstractStudying dust devils is important to better understand Mars climate and resurfacing phenomena. This paper presents an automated approach to calculate the width of tracks in orbital images. The method is based on Mathematical Morphology and was applied to a set of 200 HiRISE and MOC images of five Mars quadrangles, which were Aeolis, Argyre, Noachis, Hellas and Eridania. Information obtained by our method was compared with results of manual analysis performed by other authors. In addition, we show that track widths do not follow a normal distribution. (C) 2015 Elsevier B.V. All rights reserved.en
dc.description.affiliationInst Fed Educ Ciencia & Tecnol Mato Grosso IFMT, Belo Horizonte, MG, Brazil
dc.description.affiliationUniv Lisbon, Ctr Recursos Nat & Ambiente CERENA, IST, Ave Rovisco Pais, P-1049001 Lisbon, Portugal
dc.description.affiliationUniv Estadual Paulista, FCT, 305 Roberto Simonsen, BR-19060900 Presidente Pnidente, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, FCT, 305 Roberto Simonsen, BR-19060900 Presidente Pnidente, Brazil
dc.format.extent1-6
dc.identifierhttp://dx.doi.org/10.1016/j.aeolia.2015.11.001
dc.identifier.citationAeolian Research. Oxford: Elsevier Sci Ltd, v. 20, p. 1-6, 2016.
dc.identifier.doi10.1016/j.aeolia.2015.11.001
dc.identifier.fileWOS000372381500001.pdf
dc.identifier.issn1875-9637
dc.identifier.urihttp://hdl.handle.net/11449/165108
dc.identifier.wosWOS:000372381500001
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofAeolian Research
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.subjectMartian dust devil tracks
dc.subjectMathematical Morphology
dc.subjectAeolian process
dc.titleAutomated width measurements of Martian dust devil tracksen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.author.orcid0000-0002-8656-9147[1]
unesp.author.orcid0000-0002-3199-7961[2]
unesp.author.orcid0000-0002-7069-0479[3]
unesp.departmentCartografia - FCTpt

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