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Journal of the Optical Society of America

Journal of the Optical Society of America

  • Vol. 70, Iss. 12 — Dec. 1, 1980
  • pp: 1550–1551

Wavelength predictions for lines of interest in the Ne I sequence

S. O. Kastner  »View Author Affiliations


JOSA, Vol. 70, Issue 12, pp. 1550-1551 (1980)
http://dx.doi.org/10.1364/JOSA.70.001550


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Abstract

Recent observations and calculations, in the literature, are used to obtain estimated wavelengths of likely observable lines emitted by neonlike ions. Optimum conditions for observation are briefly discussed.

© 1980 Optical Society of America

Citation
S. O. Kastner, "Wavelength predictions for lines of interest in the Ne I sequence," J. Opt. Soc. Am. 70, 1550-1551 (1980)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-70-12-1550


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References

  1. S. O. Kastner, W. E. Behring, and L. Cohen, "Observation of subordinate 2p54d-2p53p transitions in neon-like ions from Ca XI to Ni XIX," Astrophys. J. 199, 777–780 (1975).
  2. B. C. Fawcett, G. E. Bromage, and R. W. Hayes, "Observed spectra due to n = 3 to 4 transitions in Fe XVII and isoelectronic spectra," Mon. Not. R. Astron. Soc. 186, 113–116 (1979).
  3. M. Loulergue and H. Nussbaumer, "A study of Fe XVII and Ni XIX coronal lines," Astron. Astrophys. 45, 125–134 (1975).
  4. S. O. Kastner, W. M. Neupert, and M. Swartz, "Observation of possible Fe XVII 2p53p-2p53s transitions in spectra of a solar active region and flare," Solar Phys. 43, 111–115 (1975).
  5. K. P. Dere, "Spectral lines observed in solar flares between 171 and 630 angstroms," Astrophys. J. 221, 1062–1067 (1978).
  6. L. A. Bureeva and U. I. Safronova, "Calculated lifetimes in the neon isoelectronic sequence," Phys. Scripta 20, 81–87 (1979).
  7. M. Crance, "Theoretical transition probabilities and energy levels in Ne I isoelectronic sequence," At. Data 5, 185–200 (1973).
  8. H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).
  9. S. O. Kastner, "Prediction and identification of some forbidden lines in the Ne I sequence," Solar Phys. 37, 179–181 (1974).
  10. W. E. Behring, L. Cohen, and U. Feldman, "The solar spectrum: wavelengths and identifications from 60 to 385 angstroms," Astrophys. J. 175, 493–523 (1972).
  11. W. Fielder, D. L. Lin, and D. Ton-That, "El and M2 transitions in the neon isoelectric sequence," Phys. Rev. A 19, 741–755 (1979).
  12. B. C. Fawcett, A. Ridgeley, and G. E. Bromage, "The Spectrum ArIX and extended spectral classification in ArV to ArVIII and ArX," Phys. Scripta 18, 315–322 (1978).
  13. R. J. Hutcheon, J. P. Pye, and K. D. Evans, "Weak Fe XVII transitions in the coronal x-ray spectrum," Astron. Astrophys. 51, 451–460 (1976).

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