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Please use this identifier to cite or link to this item: http://hdl.handle.net/1843/60872
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dc.creatorSantiago Andrés Trianapt_BR
dc.creatorGustavo Andres Guerrero Erasopt_BR
dc.creatorAnkit Barikpt_BR
dc.creatorJérémy Rekierpt_BR
dc.date.accessioned2023-11-13T16:49:34Z-
dc.date.available2023-11-13T16:49:34Z-
dc.date.issued2022-
dc.citation.volume934pt_BR
dc.citation.issue1pt_BR
dc.citation.spage1pt_BR
dc.citation.epage9pt_BR
dc.identifier.doihttps://doi.org/10.3847/2041-8213/ac7dacpt_BR
dc.identifier.issn2041-8213pt_BR
dc.identifier.urihttp://hdl.handle.net/1843/60872-
dc.description.resumoThe observation of global acoustic waves (p modes) in the Sun has been key to unveiling its internal structure and dynamics. A different kind of wave, known as sectoral Rossby modes, has been observed and identified, which potentially opens the door to probing internal processes that are inaccessible through p-mode helioseismology. Yet another set of waves, appearing as retrograde-propagating, equatorially antisymmetric vorticity waves, has also been observed but their identification remained elusive. Here, through a numerical model implemented as an eigenvalue problem, we provide evidence supporting the identification of those waves as a class of inertial eigenmodes, distinct from the Rossby-mode class, with radial velocities comparable to the horizontal ones deep in the convective zone but still small compared to the horizontal velocities toward the surface. We also suggest that the signature of tesseral-like Rossby modes might be present in recent observational data.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.ispartofThe Astrophysical Journal Letters-
dc.rightsAcesso Abertopt_BR
dc.subjectAstrophysical fluid dynamicspt_BR
dc.subjectSolar oscillationspt_BR
dc.subjectSolar rotationpt_BR
dc.subject.otherAstrofísicapt_BR
dc.subject.otherSolpt_BR
dc.titleIdentification of inertial modes in the solar convection zonept_BR
dc.typeArtigo de Periódicopt_BR
dc.url.externahttps://iopscience.iop.org/article/10.3847/2041-8213/ac7dacpt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-7679-3962pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0002-2671-8796pt_BR
dc.identifier.orcidhttps://orcid.org/0000-0001-5747-669Xpt_BR
dc.identifier.orcidhttps://orcid.org/0000-0003-3151-6969pt_BR
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