Composition of the Solar Interior: Information from Isotope Ratios

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dc.creatorManuel, O.
dc.creatorFriberg, Stig
dc.date2004-10-28
dc.date.accessioned2026-07-07T02:15:34Z
dc.date.available2026-07-07T02:15:34Z
dc.descriptionMeasurements are reviewed showing that the interior of the Sun, the inner planets, and ordinary meteorites consist mostly of the same elements: Iron, oxygen, nickel, silicon, magnesium, sulfur and calcium. These results do not support the standard solar model.
dc.description4 pages, includes 6 figures, 1 Table, 39 references, 2002 SOHO 12/ GONG + 2002 Conference on Local and Global Helioseismology: The Present and Future, Big Bear Lake, CA
dc.identifierhttps://arxiv.org/abs/astro-ph/0410717
dc.identifierhttp://arxiv.org/abs/astro-ph/0410717
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8457
dc.subjectAstrophysics
dc.titleComposition of the Solar Interior: Information from Isotope Ratios
dc.typetext

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