Identification of Fe I lines in the ultraviolet solar spectrum

Details Identification of Fe I lines in the ultraviolet solar spectrum Identification of Fe I lines in the ultraviolet solar spectrum

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apjs...48..437m&link_type=abstract

Astrophysical Journal Supplement Series, vol. 48, Apr. 1982, p. 437-454.

Astronomy and Astrophysics

Astrophysics

5

Iron, Line Spectra, Solar Spectra, Spectrum Analysis, Ultraviolet Spectra, Data Reduction, Rocket-Borne Instruments, Solar Limb, Tables (Data)

Scientific paper

High-resolution ultraviolet echelle spectrograms of the sun obtained from a rocket-borne spectrograph have been used for the identification of Fe I absorption lines in the wavelength range 1770-2020 A. Wavelength measurements, with a precision of about 15 mA, are tabulated for 425 Fe I features, along with available laboratory wavelenghs or predicted wavelengths calculated from atomic energy level data. The classification system of Moore has been extended to include possible additional multiplets with 126 newly classified lines; 234 unclassified lines were observed and identified with laboratory Fe I spectra

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