Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/12216
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dc.date.accessioned2019-02-01T13:53:38Zen
dc.date.available2019-02-01T13:53:38Zen
dc.date.issued2019-
dc.identifier.urihttp://hdl.handle.net/2122/12216en
dc.description.abstractThis study proposes a model to explain the Martian phenomenon of gullies. Starting from the geomorphological evidence we want to assess the possibility that water plays a primary role in the origin of gullies. A role exercised at current climatic conditions.en_US
dc.description.sponsorshipINGVen_US
dc.language.isoEnglishen_US
dc.subjectMars, gullies, wateren_US
dc.titlePhysics of the martian gullies from geomorphological evidenceen_US
dc.typearticleen_US
dc.description.statusNot submitteden_US
dc.type.QualityControlUnreferreden_US
dc.subject.INGV02.01. Permafrosten_US
dc.description.obiettivoSpecifico2TM. Divulgazione Scientificaen_US
dc.description.journalTypeN/A or not JCRen_US
dc.contributor.authorNardi, Adriano-
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen_US
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.orcid0000-0002-7211-2963-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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