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

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  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).

1979 (3)

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).

L. A. Bureeva and U. I. Safronova, "Calculated lifetimes in the neon isoelectronic sequence," Phys. Scripta 20, 81–87 (1979).

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).

1978 (3)

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).

H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).

K. P. Dere, "Spectral lines observed in solar flares between 171 and 630 angstroms," Astrophys. J. 221, 1062–1067 (1978).

1976 (1)

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).

1975 (3)

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).

M. Loulergue and H. Nussbaumer, "A study of Fe XVII and Ni XIX coronal lines," Astron. Astrophys. 45, 125–134 (1975).

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).

1974 (1)

S. O. Kastner, "Prediction and identification of some forbidden lines in the Ne I sequence," Solar Phys. 37, 179–181 (1974).

1973 (1)

M. Crance, "Theoretical transition probabilities and energy levels in Ne I isoelectronic sequence," At. Data 5, 185–200 (1973).

1972 (1)

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).

Baudinet-Robinet, Y.

H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).

Behring, W. E.

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).

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).

Bromage, G. E.

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).

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).

Bureeva, L. A.

L. A. Bureeva and U. I. Safronova, "Calculated lifetimes in the neon isoelectronic sequence," Phys. Scripta 20, 81–87 (1979).

Cohen, L.

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).

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).

Crance, M.

M. Crance, "Theoretical transition probabilities and energy levels in Ne I isoelectronic sequence," At. Data 5, 185–200 (1973).

Dere, K. P.

K. P. Dere, "Spectral lines observed in solar flares between 171 and 630 angstroms," Astrophys. J. 221, 1062–1067 (1978).

Dumont, P. D.

H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).

Evans, K. D.

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).

Fawcett, B. C.

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).

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).

Feldman, U.

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).

Fielder, W.

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).

Garnir, H. P.

H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).

Hayes, R. W.

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).

Hutcheon, R. J.

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).

Kastner, S. O.

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).

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).

S. O. Kastner, "Prediction and identification of some forbidden lines in the Ne I sequence," Solar Phys. 37, 179–181 (1974).

Lin, D. L.

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).

Loulergue, M.

M. Loulergue and H. Nussbaumer, "A study of Fe XVII and Ni XIX coronal lines," Astron. Astrophys. 45, 125–134 (1975).

Neupert, W. M.

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).

Nussbaumer, H.

M. Loulergue and H. Nussbaumer, "A study of Fe XVII and Ni XIX coronal lines," Astron. Astrophys. 45, 125–134 (1975).

Pye, J. P.

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).

Ridgeley, A.

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).

Safronova, U. I.

L. A. Bureeva and U. I. Safronova, "Calculated lifetimes in the neon isoelectronic sequence," Phys. Scripta 20, 81–87 (1979).

Swartz, M.

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).

Ton-That, D.

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).

Astron. Astrophys. (2)

M. Loulergue and H. Nussbaumer, "A study of Fe XVII and Ni XIX coronal lines," Astron. Astrophys. 45, 125–134 (1975).

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).

Astrophys. J. (3)

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).

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).

K. P. Dere, "Spectral lines observed in solar flares between 171 and 630 angstroms," Astrophys. J. 221, 1062–1067 (1978).

At. Data (1)

M. Crance, "Theoretical transition probabilities and energy levels in Ne I isoelectronic sequence," At. Data 5, 185–200 (1973).

Mon. Not. R. Astron. Soc. (1)

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).

Phys. Rev. A (1)

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).

Phys. Scripta (3)

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).

H. P. Garnir, Y. Baudinet-Robinet, and P. D. Dumont, "Study of SVII in the vacuum ultraviolet," Phys. Scripta 17, 463–465 (1978).

L. A. Bureeva and U. I. Safronova, "Calculated lifetimes in the neon isoelectronic sequence," Phys. Scripta 20, 81–87 (1979).

Solar Phys. (2)

S. O. Kastner, "Prediction and identification of some forbidden lines in the Ne I sequence," Solar Phys. 37, 179–181 (1974).

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).

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