Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Oxford University, Oxford, England
Sandia Laboratories, Albuquerque, N. Mex.
Analysis of Fe I lines /chi between 0.00 eV. and 2.6 eV/ in the solar spectrum using improved damping constants and accurate oscillator strengths - Test of a solar model atmosphere
Comments concerning the Kallmann-White-Newell Article, "Physical Properties of the Atmosphere from 90 to 300 Kilometers"
Interpretation of TI I lines of excitation energy 0.0-0.05 eV in the solar spectrum - Use of new oscillator strengths of accuracy 0.5 per cent
Measurement of relative oscillator strengths for Fe I: Transitions from levels /b-3/-F/2-4/ /2.61 eV-2.56 eV/ - Use of a multipass optical system
Note on the interpretation of Fe I lines /2.18-2.49 eV/ in the solar spectrum
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