Precision measurement of relative oscillator strengths. V - Comparison of oscillator strengths of Fe I transitions from levels a5 F/1-5/ /0.86-1.01 eV/ and those from a5 D/0-4/ /0.00-0.12 eV/

Details Precision measurement of relative oscillator strengths. V - Comparison of oscillator strengths of Fe I transitions from levels a5 F/1-5/ /0.86-1.01 eV/ and those from a5 D/0-4/ /0.00-0.12 eV/ Precision measurement of relative oscillator strengths. V - Comparison of oscillator strengths of Fe I transitions from levels a5 F/1-5/ /0.86-1.01 eV/ and those from a5 D/0-4/ /0.00-0.12 eV/

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..651a&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Mar. 1979, p. 651-655. Research supported by the Science Research

Astronomy and Astrophysics

Astronomy

20

Astronomical Spectroscopy, Atomic Excitations, Atomic Spectra, Iron, Oscillators, Absorption Spectra, Furnaces, Line Spectra, Pyrometers, Spectral Line Width

Scientific paper

A photoelectric pyrometer has been built and used to measure the temperature of the Oxford spectroscopic furnace on the International Practical Temperature Scale 1968 to an accuracy of + or - 1 K (3 sigma). Measurements have been made of the relative oscillator strengths of Fe I absorption lines originating from energy levels separated by about 1 eV. These measures have an accuracy of about 0.5 percent and are intended to link existing measures made at Oxford from levels a5 F(1-5) (0.86-1.01 eV) to measures made from levels a5 D(0-4) (0.00-0.12 eV).

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