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Oscillator Strengths from the High S/N Solar Spectrum

Published online by Cambridge University Press:  19 July 2016

Robert J. Rutten
Robert J. Rutten*
Affiliation:
Utrecht Observatory, The Netherlands

Extract

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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.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 367 - 371
Copyright
Copyright © Kluwer 1988 

References

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