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Venus diapirs: Thermal of compositional?

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dc.contributor.authorHansen, V
dc.date.accessioned2015-12-13T23:14:07Z
dc.date.available2015-12-13T23:14:07Z
dc.date.issued2003
dc.date.updated2015-12-12T08:37:00Z
dc.description.abstractThe Venus surface exhibits quasi-circular structures with a bimodal size distribution; there are at least 17 large (∼1300-2600-km diameter) crustal plateaus and volcanic rises, which form major geomorphic features, and ∼515 smaller (200-km median diam
dc.identifier.issn0016-7606
dc.identifier.urihttp://hdl.handle.net/1885/88448
dc.publisherAssociation of Engineering Geologists
dc.sourceGeological Society of America Bulletin
dc.subjectKeywords: Lithosphere; Boundary layers; Buoyancy; Heat transfer; Thermal plumes; Geomorphology; corona; diapir; planetary surface; plume; thermal evolution; Venus Coronae; Diaper; Plume; Thermal evolution; Venus
dc.titleVenus diapirs: Thermal of compositional?
dc.typeJournal article
local.bibliographicCitation.issue9
local.bibliographicCitation.lastpage1052
local.bibliographicCitation.startpage1040
local.contributor.affiliationHansen, V, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidHansen, V, u3446135
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor040403 - Geophysical Fluid Dynamics
local.identifier.ariespublicationMigratedxPub18139
local.identifier.citationvolume115
local.identifier.doi10.1130/B25155.1
local.identifier.scopusID2-s2.0-0141795492
local.type.statusPublished Version

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