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Image processing algorithm for the identification of Martian dust devil tracks in MOC and HiRISE images

dc.contributor.authorStatella, Thiago
dc.contributor.authorPina, Pedro
dc.contributor.authorSilva, Erivaldo Antonio da [UNESP]
dc.contributor.institutionIFMT
dc.contributor.institutionIST
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T13:22:37Z
dc.date.available2014-05-20T13:22:37Z
dc.date.issued2012-09-01
dc.description.abstractThis paper presents a method for automatic identification of dust devils tracks in MOC NA and HiRISE images of Mars. The method is based on Mathematical Morphology and is able to successfully process those images despite their difference in spatial resolution or size of the scene. A dataset of 200 images from the surface of Mars representative of the diversity of those track features was considered for developing, testing and evaluating our method, confronting the outputs with reference images made manually. Analysis showed a mean accuracy of about 92%. We also give some examples on how to use the results to get information about dust devils, namelly mean width, main direction of movement and coverage per scene. (c) 2012 Elsevier Ltd. All rights reserved.en
dc.description.affiliationIFMT, Inst Fed Educ Ciência & Tecnol Mato Grosso, BR-78002520 Cuiaba, Brazil
dc.description.affiliationIST, Ctr Recursos Nat & Ambiente CERENA, P-1049001 Lisbon, Portugal
dc.description.affiliationUniv Estadual Paulista, FCT, BR-19060900 Presidente Prudente, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, FCT, BR-19060900 Presidente Prudente, Brazil
dc.format.extent46-58
dc.identifierhttp://dx.doi.org/10.1016/j.pss.2012.06.003
dc.identifier.citationPlanetary and Space Science. Oxford: Pergamon-Elsevier B.V. Ltd, v. 70, n. 1, p. 46-58, 2012.
dc.identifier.doi10.1016/j.pss.2012.06.003
dc.identifier.issn0032-0633
dc.identifier.lattes9103545004507135
dc.identifier.orcid0000-0002-7069-0479
dc.identifier.urihttp://hdl.handle.net/11449/6670
dc.identifier.wosWOS:000308386900005
dc.language.isoeng
dc.publisherPergamon-Elsevier B.V. Ltd
dc.relation.ispartofPlanetary and Space Science
dc.relation.ispartofjcr1.820
dc.relation.ispartofsjr1,065
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectDust devilsen
dc.subjectFeature detectionen
dc.subjectMathematical Morphologyen
dc.subjectMarsen
dc.titleImage processing algorithm for the identification of Martian dust devil tracks in MOC and HiRISE imagesen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderPergamon-Elsevier B.V. Ltd
dspace.entity.typePublication
unesp.author.lattes9103545004507135
unesp.author.orcid0000-0002-7069-0479[3]
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Ciências e Tecnologia, Presidente Prudentept
unesp.departmentCartografia - FCTpt

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