A number of wave functions for bound electrons have been calculated in scaled Thomas-Fermi ion potentials in order to evaluate some oscillator strengths and mean square radii. The results differ only slightly from those obtained by the well-known method of Bates and Damgaard. After that, the values of the oscillator strengths for the transition 4 s→4 p in Si i have been evaluated in intermediate coupling, showing large differences with the LS-coupling results. These new values are supported by the fact that they show somewhat better agreement with observations, described earlier in this issue of Solar Physics by De Jager and Neven. © 1970 D. Reidel Publishing Company.SCOPUS: ar.jinfo:eu-repo/semantics/publishe
Regularities in the distribution of oscillator strengths of lines in spectra of alkali metal atoms a...
The atomic quantities for bound-bound transitions such as the oscillator strengths, the line strengt...
Context. Transition lines of neutral calcium are observed in the spectra of stellar and substellar o...
An extensive dataset of oscillator strengths, line strengths, and Einstein A-coefficients has been c...
Energy levels and oscillator strengths (transition probabilities) have been calculated for transitio...
The atomic quantities for bound-bound transitions such as the oscillator strengths, the line strengt...
Aims. Oscillator strengths and electron impact excitation collision strengths for transitions betwee...
An extensive dataset of oscillator strengths, line strengths, and Einstein A-coefficients has been c...
Because they play a fundamental role in the calculation of bound electron stopping-powers, photon me...
Oscillator strengths and radiative transition probabilities for dipole allowed fine structure levels...
Oscillator strengths and radiative transition probabilities for dipole allowed fine structure levels...
Photoionization cross sections, oscillator strengths and energy levels of the silicon-like ions, Si^...
There is an on-going need for accurate oscillator strengths to be used in astrophysical applications...
Aims. This work reports on radiative transition rates and electron impact excitation collision stren...
Monthly Notices of the Royal Astronomical Society, 372, pp. 609-614, http://dx.doi.org./10.1111/j.13...
Regularities in the distribution of oscillator strengths of lines in spectra of alkali metal atoms a...
The atomic quantities for bound-bound transitions such as the oscillator strengths, the line strengt...
Context. Transition lines of neutral calcium are observed in the spectra of stellar and substellar o...
An extensive dataset of oscillator strengths, line strengths, and Einstein A-coefficients has been c...
Energy levels and oscillator strengths (transition probabilities) have been calculated for transitio...
The atomic quantities for bound-bound transitions such as the oscillator strengths, the line strengt...
Aims. Oscillator strengths and electron impact excitation collision strengths for transitions betwee...
An extensive dataset of oscillator strengths, line strengths, and Einstein A-coefficients has been c...
Because they play a fundamental role in the calculation of bound electron stopping-powers, photon me...
Oscillator strengths and radiative transition probabilities for dipole allowed fine structure levels...
Oscillator strengths and radiative transition probabilities for dipole allowed fine structure levels...
Photoionization cross sections, oscillator strengths and energy levels of the silicon-like ions, Si^...
There is an on-going need for accurate oscillator strengths to be used in astrophysical applications...
Aims. This work reports on radiative transition rates and electron impact excitation collision stren...
Monthly Notices of the Royal Astronomical Society, 372, pp. 609-614, http://dx.doi.org./10.1111/j.13...
Regularities in the distribution of oscillator strengths of lines in spectra of alkali metal atoms a...
The atomic quantities for bound-bound transitions such as the oscillator strengths, the line strengt...
Context. Transition lines of neutral calcium are observed in the spectra of stellar and substellar o...