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Analysis of Very High Excitation Fe I Lines (4f–5g) in the Solar Infrared Spectrum
Published online by Cambridge University Press: 03 August 2017
Abstract
We present a detailed analysis of very high excitation lines (4f–5g) of Fe I which are present in the spectral region 2545–2585 cm–1 in high resolution spectra both in the laboratory and in the ATMOS solar spectra obtained from space. A value of the solar abundance of iron which agrees with the meteoritic value is derived.
- Type
- Part 6: The Infrared Spectrum
- Information
- Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 543 - 548
- Copyright
- Copyright © Kluwer 1994