The seismic structure of the sun

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 i...

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Detalhes bibliográficos
Autor principal: Gough, DO (author)
Outros Autores: Kosovichev, AG (author), Toomre, J (author), Anderson, E (author), Antia, HM (author), Basu, S (author), Chaboyer, B (author), Chitre, SM (author), ChristensenDalsgaard, J (author), Dziembowski, WA (author), EffDarwich, A (author), Elliott, JR (author), Giles, PM (author), Goode, PR (author), Guzik, JA (author), Harvey, JW (author), Hill, F (author), Leibacher, JW (author), Monteiro, MJPFG (author), Richard, O (author), Sekii, T (author), Shibahashi, T (author), Takata, M (author), Thompson, MJ (author), Vauclair, S (author), Vorontsov, SV (author)
Formato: article
Idioma:eng
Publicado em: 1996
Assuntos:
Astronomia
Astronomy
Texto completo:https://repositorio-aberto.up.pt/handle/10216/100614
País:Portugal
Oai:oai:repositorio-aberto.up.pt:10216/100614

Texto Completo

https://repositorio-aberto.up.pt/handle/10216/100614

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