Abundances of the rare earths in the sun

N. Grevesse, G. Blanquet

Résultats de recherche: Contribution à un journal/une revueArticle

Résumé

We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.
langueAnglais
Pages5-17
Nombre de pages13
journalSolar Physics
Volume8
Numéro1
Les DOIs
étatPublié - 1 juil. 1969

Empreinte digitale

sun
rare earth elements
solar spectra
meteorites
tracing
nuclear fusion
Switzerland
meteorite
stations
high resolution
station

Citer ceci

Grevesse, N. ; Blanquet, G./ Abundances of the rare earths in the sun. Dans: Solar Physics. 1969 ; Vol 8, Numéro 1. p. 5-17
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Abundances of the rare earths in the sun. / Grevesse, N.; Blanquet, G.

Dans: Solar Physics, Vol 8, Numéro 1, 01.07.1969, p. 5-17.

Résultats de recherche: Contribution à un journal/une revueArticle

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AU - Blanquet,G.

N1 - Copyright 2007 Elsevier B.V., All rights reserved.

PY - 1969/7/1

Y1 - 1969/7/1

N2 - We have determined the solar abundances of the rare earths (La, Ce, Pr, Nd, Sm, Eu, Gd, Dy, Er, Tm, Yb, Lu) on the basis of measurements made on new high-resolution tracings of the solar spectrum obtained at the International Scientific Station of the Jungfraujoch (Switzerland) by L. Delbouille, L. Neven and G. Roland. Our results (Table XV) are compared with those of other authors for the sun and meteorites as well as with the abundances predicted by nucleosynthesis theories.

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Grevesse N, Blanquet G. Abundances of the rare earths in the sun. Solar Physics. 1969 juil. 1;8(1):5-17. Disponible �, DOI: 10.1007/BF00150651