Use este identificador para citar ou linkar para este item: http://hdl.handle.net/1843/60872
Tipo: Artigo de Periódico
Título: Identification of inertial modes in the solar convection zone
Autor(es): Santiago Andrés Triana
Gustavo Andres Guerrero Eraso
Ankit Barik
Jérémy Rekier
Resumo: The 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.
Assunto: Astrofísica
Sol
Idioma: eng
País: Brasil
Editor: Universidade Federal de Minas Gerais
Sigla da Instituição: UFMG
Departamento: ICX - DEPARTAMENTO DE FÍSICA
Tipo de Acesso: Acesso Aberto
Identificador DOI: https://doi.org/10.3847/2041-8213/ac7dac
URI: http://hdl.handle.net/1843/60872
Data do documento: 2022
metadata.dc.url.externa: https://iopscience.iop.org/article/10.3847/2041-8213/ac7dac
metadata.dc.relation.ispartof: The Astrophysical Journal Letters
Aparece nas coleções:Artigo de Periódico

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