Interpretation of the solar spectrum 300 NM to 900 nm. I - Fe I lines of excitation potential 0.00 eV-0.12 eV microturbulence, damping, abundance, tests of oscillator strengths

Details Interpretation of the solar spectrum 300 NM to 900 nm. I - Fe I lines of excitation potential 0.00 eV-0.12 eV microturbulence, damping, abundance, tests of oscillator strengths Interpretation of the solar spectrum 300 NM to 900 nm. I - Fe I lines of excitation potential 0.00 eV-0.12 eV microturbulence, damping, abundance, tests of oscillator strengths

Oct 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.177..227b&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 177, Oct. 1976, p. 227-245.

Astronomy and Astrophysics

Astronomy

47

Iron, Line Spectra, Solar Spectra, Spectrum Analysis, Absorption Spectra, Atmospheric Turbulence, Solar Atmosphere, Turbulence Effects

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1976MNRAS.177..227B

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