Wet Mars implications of revised scaling calculations for Evros Vallis

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dc.contributor.authorCaprarelli, Graziella
dc.contributor.authorWang, B. Y.
dc.date.accessioned2015-12-13T22:19:19Z
dc.date.issued2012
dc.date.updated2016-02-24T09:03:03Z
dc.description.abstractIn this paper we report the results of our investigation of Evros Vallis, a martian late Noachian dendritic valley network centered at ~12°E, 12°S. The study area is located SSW of Schiaparelli and SE relative to Meridiani Planum. After establishment of
dc.identifier.issn0812-0099
dc.identifier.urihttp://hdl.handle.net/1885/71736
dc.publisherBlackwell Publishing Ltd
dc.sourceAustralian Journal of Earth Sciences
dc.subjectKeywords: altimetry; digital elevation model; erosion rate; geomorphological response; image analysis; landscape evolution; Mars; morphometry; observational method; planetary atmosphere; planetary landform; planetary surface; tectonic setting; valley; water content climate; DEM; Mars; MOLA; scaling; valley networks
dc.titleWet Mars implications of revised scaling calculations for Evros Vallis
dc.typeJournal article
local.bibliographicCitation.issue2
local.bibliographicCitation.lastpage276
local.bibliographicCitation.startpage263
local.contributor.affiliationCaprarelli, Graziella, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWang, B. Y., University of Technology
local.contributor.authoruidCaprarelli, Graziella, u5036215
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor049999 - Earth Sciences not elsewhere classified
local.identifier.ariespublicationf5625xPUB2855
local.identifier.citationvolume59
local.identifier.doi10.1080/08120099.2012.622294
local.identifier.scopusID2-s2.0-84859360839
local.type.statusPublished Version

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