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Scientist
Oxford University, Oxford, England
Oxford University, England
An LTE analysis of the solar photospheric TI I and CR I Spectra - Evidence for non-LTE in excitation
Empirical improvement in accuracy of atomic oscillator strengths calculated by Kurucz and Peytremann
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. II - Measures for transitions from levels with excitation energy 2.54-3.46 eV
Measurement of relative oscillator strengths for TI I. III Weak transitions from levels a3F(3, 4) (0.02 eV, 0.05 eV), a5F(1-5) (0.81 eV-0.85 eV), a1D(2) (0.90 eV), a3P(0-3) (1.05 eV-1.07 eV) with solar analysis
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