Abundances in the solar corona

Computer Science

Scientific paper

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Solar Corona, Stellar Spectra, Plasma Composition, Ionization Potentials, Abundance, Temperature Dependence

Scientific paper

The present survey of recent work on solar coronal abundances encompasses analyses of stellar spectra and emphasized the question as to the accuracy of atomic data, especially the temperature-dependence of ionization fractions. It is noted that inaccuracies significantly affect the derived abundances sufficiently to mask any variations that may exist in the first ionization potential.

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