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dc.contributor.authorGarcia, F.
dc.contributor.authorOruba, L.
dc.contributor.authorDormy, E.
dc.date.accessioned2017-02-08T14:36:50Z
dc.date.available2017-02-08T14:36:50Z
dc.date.issued2016-06-27
dc.identifier.urihttp://hdl.handle.net/2117/100691
dc.format.extent1 p.
dc.language.isoeng
dc.publisherUniversitat Politècnica de Catalunya
dc.relation.ispartofEuropean GyR Dynamo (2016: Barcelona)
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshDynamo theory (Cosmic physics)
dc.titleDipolar to non-dipolar transition and equatorial symmetry breaking in rotating spherical shells. Influence of the Prandtl number
dc.typeConference report
dc.subject.lemacDinamo, Teoria (Física còsmica)
dc.rights.accessOpen Access


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