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The seismic structure of the sun

Gough, DO; Kosovichev, AG; Toomre, J; Anderson, E; Antia, HM; Basu, S; Chaboyer, B; Chitre, SM; ChristensenDalsgaard, J; Dziembowski, WA; EffDarwich, A

Global Oscillation Network Group data reveal that the internal structure of the sun can be well represented by a calibrated standard model. However, immediately beneath the convection zone and at the edge of the energy-generating core, the sound-speed variation is somewhat smoother in the sun than it is in the model. This could be a consequence of chemical inhomogeneity that is too severe in the model, perhaps ...

Date: 1996 | Origin: Repositório Aberto da Universidade do Porto

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