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Please use this identifier to cite or link to this item: http://hdl.handle.net/1843/60334
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dc.creatorGustavo Andres Guerrero Erasopt_BR
dc.date.accessioned2023-10-31T15:04:10Z-
dc.date.available2023-10-31T15:04:10Z-
dc.date.issued2019-
dc.citation.volume15pt_BR
dc.citation.issue354pt_BR
dc.citation.spage65pt_BR
dc.citation.epage85pt_BR
dc.identifier.doihttps://doi.org/10.1017/S1743921320000721pt_BR
dc.identifier.issn1743-9221pt_BR
dc.identifier.urihttp://hdl.handle.net/1843/60334-
dc.description.resumoThe dynamo mechanism, responsible for the solar magnetic activity, is still an open problem in astrophysics. Different theories proposed to explain such phenomena have failed in reproducing the observational properties of the solar magnetism. Thus, ab-initio computational modeling of the convective dynamo in a spherical shell turns out as the best alternative to tackle this problem. In this work we review the efforts performed in global simulations over the past decades. Regarding the development and sustain of mean-flows, as well as mean magnetic field, we discuss the points of agreement and divergence between the different modeling strategies. Special attention is given to the implicit large-eddy simulations performed with the EULAG-MHD code.pt_BR
dc.format.mimetypepdfpt_BR
dc.languageengpt_BR
dc.publisherUniversidade Federal de Minas Geraispt_BR
dc.publisher.countryBrasilpt_BR
dc.publisher.departmentICX - DEPARTAMENTO DE FÍSICApt_BR
dc.publisher.initialsUFMGpt_BR
dc.relation.ispartofProceedings of the International Astronomical Union-
dc.rightsAcesso Abertopt_BR
dc.subjectSunpt_BR
dc.subjectStarspt_BR
dc.subjectMagnetic fieldspt_BR
dc.subject.otherSolpt_BR
dc.subject.otherEstrelaspt_BR
dc.subject.otherCampos magnéticospt_BR
dc.titleGlobal simulations of stellar dynamospt_BR
dc.typeArtigo de Periódicopt_BR
dc.url.externahttps://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/global-simulations-of-stellar-dynamos/1B61CE1D4ED9C59B86A070734EC214C3pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-2671-8796pt_BR
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