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Oscillator Strengths from the High S/N Solar Spectrum
Published online by Cambridge University Press: 19 July 2016
Extract
Most of modern solar physics is not concerned with high S/N spectrometry, but rather with high spatial resolution in narrow-band imaging as well as spectrometry, and with high Fourier resolution in helioseismology.
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- VI. Chemical Composition of Stars
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- Copyright © Kluwer 1988