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Standard Solar Composition

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Solar Composition and its Evolution — from Core to Corona

Part of the book series: Space Sciences Series of ISSI ((SSSI,volume 5))

Abstract

We review the current status of our knowledge of the chemical composition of the Sun, essentially derived from the analysis of the solar photospheric spectrum. The comparison of solar and meteoritic abundances confirms that there is a very good agreement between the two sets of abundances. They are used to construct a Standard Abundance Distribution.

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Abbreviations

CI:

Carbonaceous Chondrite

SW:

Solar Wind

SEP:

Solar Energetic Particles

SAD:

Standard Abundance Distribution

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Author information

Authors and Affiliations

  1. Institut d’Astrophysique et de Géophysique, Université de Liège, 5, Avenue de Cointe, B-4000, Liège, Belgium

    N. Grevesse & A. J. Sauval

  2. Observatoire Royal de Belgique, B-1180, Bruxelles, Belgium

    N. Grevesse & A. J. Sauval

Authors
  1. N. Grevesse
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  2. A. J. Sauval
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Editor information

Editors and Affiliations

  1. Physikalisch-meteorologisches Observatorium, World Radiation Center, Davos, Switzerland

    C. Fröhlich

  2. Space Science Department of ESA, ESTEC, Noordwijk, The Netherlands

    M. C. E. Huber

  3. Institute of Astronomy, ETH, Zürich, Switzerland

    S. K. Solanki

  4. International Space Science Institute, Bern, Switzerland

    R. Von Steiger

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© 1998 Springer Science+Business Media Dordrecht

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Grevesse, N., Sauval, A.J. (1998). Standard Solar Composition. In: Fröhlich, C., Huber, M.C.E., Solanki, S.K., Von Steiger, R. (eds) Solar Composition and its Evolution — from Core to Corona. Space Sciences Series of ISSI, vol 5. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4820-7_15

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  • DOI: https://doi.org/10.1007/978-94-011-4820-7_15

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6022-6

  • Online ISBN: 978-94-011-4820-7

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