Photospheric abundances

Details Photospheric abundances Photospheric abundances

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.348..305g&link_type=abstract

In ESA, Proceedings of the First SOHO Workshop: Coronal Streamers, Coronal Loops, and Coronal and Solar Wind Composition p 305-3

Computer Science

52

Chemical Composition, Photosphere, Solar Corona, Sun, Abundance, Energetic Particles, Line Spectra, Solar Spectra, Solar Wind, Spectrum Analysis

Scientific paper

The photospheric abundances of the chemical elements which are observed in the coronal spectrum, in the solar wind and in solar energetic particle events, are reviewed. Elements which can be measured in the solar upper layers and whose abundances were revised since Anders and Grevess are discussed: helium, neon argon, iron, carbon nitrogen oxygen, fluorine chlorine, scandium titanium.

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