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Fabry-Pérot interferograms of the solar Mgii resonance lines
Published online by Cambridge University Press: 14 August 2015
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The resonance lines of Mgii occur at wavelengths (2802.7 Å, 2795.5 Å) just beyond the extinction limit of the Earth's atmosphere. At such wavelengths sophisticated optical techniques can now be employed and this fact, together with the high cosmic abundance of magnesium, makes these lines particularly important for study in UV Astronomy. In the case of the Sun, the lines consist of a broad absorption with a pronounced emission core.
- Type
- Part II: Stellar Line Spectra
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- Copyright
- Copyright © Reidel 1970
References
Purcell, J. D., Garrett, D. L., and Tousey, R.: 1962, in Space Research, vol. III, p. 781.Google Scholar