Fe I line shifts in the Sun (Allende Prieto+ 1998)

Details Fe I line shifts in the Sun (Allende Prieto+ 1998) Fe I line shifts in the Sun (Allende Prieto+ 1998)

Sep 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ycat..41290041a&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/129/41. Originally published in: 1998A&AS..129...41A

Physics

Atomic Physics

Sun, Atomic Physics

Scientific paper

Central wavelengths measured in the FTS disc-centre spectrum, in the FTS flux spectrum, rest wavelengths, excitation potentials, transition probabilities (log(gfs)) and line equivalent widths at the centre of the disc when available (from Moore et al. 1966 (The Solar Spectrum 2935Å to 8770Å, National Bureau of Standards Monograph 61) and compiled by A. D. Wittmann, private communication). An asterisk in the equivalent width means that the line has a blend.
(1 data file).

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