Models of solar surface dynamics: Impact on eigenfrequencies and radius

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dc.contributor.authorPiau, L
dc.contributor.authorCollet, Remo
dc.contributor.authorStein, R. F.
dc.contributor.authorTrampedach, Regner
dc.contributor.authorMorel, P
dc.contributor.authorTurck-Chièze, S
dc.date.accessioned2015-12-13T22:39:44Z
dc.date.issued2014
dc.date.updated2015-12-11T09:51:55Z
dc.description.abstractWe study the effects of different descriptions of the solar surface convection on the eigenfrequencies of p modes. 1D evolution calculations of the whole Sun and 3D hydrodynamic and magnetohydrodynamic simulations of the current surface are performed. The
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/77906
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleModels of solar surface dynamics: Impact on eigenfrequencies and radius
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage175
local.bibliographicCitation.startpage164
local.contributor.affiliationPiau, L, Avenue de Italie
local.contributor.affiliationCollet, Remo, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationStein, R. F., Michigan State University
local.contributor.affiliationTrampedach, Regner, University of Colorado
local.contributor.affiliationMorel, P, Observatoire de la Cote d’Azur
local.contributor.affiliationTurck-Chièze, S, CEA Saclay
local.contributor.authoremailu5236916@anu.edu.au
local.contributor.authoruidCollet, Remo, u5236916
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB6643
local.identifier.citationvolume437
local.identifier.doi10.1093/mnras/stt1866
local.identifier.scopusID2-s2.0-84890032403
local.identifier.thomsonID000328373000034
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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