Wavelengths and classifications of emission lines due to 2s22pn−2s2pn + 1 and 2s2pn−2pn + 1 transitions, Z ≤ 28

This publication has 11 references indexed in Scilit:

• The Identification of Solar Flare Fe XVIII to Fe XXIII Emission Lines FromFormulaTransitions
  Monthly Notices of the Royal Astronomical Society, 1975
• Z-dependence of the level intervals in 2s 2 2p 2, 2s 2 2p 3 and 2s 2 2p 4
  Solar Physics, 1972
• The identification of new forbidden coronal lines in the solar EUV spectrum
  Solar Physics, 1971
• Rocket Observations of the Ultraviolet Solar Spectrum during the Total Eclipse of 1970 March 7
  The Astrophysical Journal, 1971
• Plasma light sources
  Nuclear Instruments and Methods, 1970
• On the identification of Ar x and Ar xiv in the solar corona and the origin of the unidentified coronal lines
  Solar Physics, 1969
• Spin-forbidden resonance multiplets in light elements
  Solar Physics, 1969
• Theoretical Calculation of Atomic Spectra Using Digital Computers*
  Journal of the Optical Society of America, 1968
• Atomic Self-Consistent-Field Calculations Using Statistical Approximations for Exchange and Correlation
  Physical Review B, 1967
• Wavelength measurements in the vacuum ultra-violet
  Reports on Progress in Physics, 1963