Measurement of relative oscillator strengths for CR I lines. I - Measures for transitions from levels a7S3(0.00eV), a5S2(0.94eV) and a5D0-4(0.96-1.03eV)

Details Measurement of relative oscillator strengths for CR I lines. I - Measures for transitions from levels a7S3(0.00eV), a5S2(0.94eV) and a5D0-4(0.96-1.03eV) Measurement of relative oscillator strengths for CR I lines. I - Measures for transitions from levels a7S3(0.00eV), a5S2(0.94eV) and a5D0-4(0.96-1.03eV)

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.207..533b&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 207, April 1, 1984, p. 533-546. Research supported by t

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47

Astronomical Spectroscopy, Chromium, Line Spectra, Oscillator Strengths, Electron Transitions, Solar Spectra

Scientific paper

Relative oscillator strengths of 49 lines of Cr I with excitation energies of up to 1.03 volts have been measured using the Oxford spectroscopic furnace to an accuracy of better than 1 percent. Where direct relative measurements could not be made because of the largeness of the ratios of oscillator strengths, the values obtained by Huber and Sandeman (1977) using the hook method were adopted. The relative measures are placed on an absolute scale using lifetime data, and comparisons are made with data from other authors.

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