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Structure of Atomic Spectra: Some Recent Laboratory Research of Interest for Stellar Spectroscopy

Published online by Cambridge University Press:  30 March 2016

William C. Martin*
Affiliation:
National Bureau of Standards, Washington, D.C. 20234

Extract

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The data covered are wavelength, line classifications, and energy levels, and the references (numbers in brackets) are mainly supplementary to those supplied by Working Group 4 for the 1982 Report of Commission 14.

New compilations of the energy levels for all the spectra of Fe (Fe I - XXVI) [42] and Co (Co I - XXVII) [43] have been published. Although compilations of the levels for the 235 iron-group spectra (K through Ni) by the NBS AEL Data Center have been published by element during the past five years, the single-volume collection of these levels now under preparation will incorporate fairly extensive additions and revisions for many of the spectra. A compilation of the levels for Si (Si I – XIV) has been completed and should appear early in 1983.

Type
Joint Commission Meetings
Copyright
Copyright © Reidel 1983

References

[1] Mazzoni, M., Tozzl, G.P., Cantù, A.M., and Pettlni, M.: 1981, Physica 111 C, pp. 379385.Google Scholar
[2] Okasaka, R. and Fukuda, K.: 1982, J. Phys. B 15, pp. 347355.Google Scholar
[3] Huldt, S., Johansson, S., Litzén, U., and Wyart, J.F.: 1982, Phys. Scr. 25, pp. 401412.Google Scholar
[4] Ekberg, J.O. and Engstrom, L.: 1982, Phys. Scr. 25, pp. 611622.Google Scholar
[5] Johansson, S., Physics Department, University of Lund, Sweden, work in progress.Google Scholar
[6] Svendenlus, N.: 1980, Phys, Scr. 22, pp. 240287.Google Scholar
[7] Svendenlus, N.: 1980, Phys. Scr. 22, >pp. 288293.pp.+288–293.>Google Scholar
[8] Johansson, S. and Litzén, U.: 1980, Phys. Scr. 22, pp. 4960. This paper was cited as ref. 42 in the report [57] but a wrong reference number was given after Sc II In Table 1.Google Scholar
[9] Kaufman, V., Sugar, J., and Cooper, D.: 1982, Phys. Scr. 25, pp. 623626.Google Scholar
[10] Kaufman, V., Sugar, J. and Cooper, D.: 1982, Phys. Scr. 26, (In press).Google Scholar
[11] Sugar, J., Kaufman, V., and Cooper, D.: 1982, Phys. Scr. 26, (In press).Google Scholar
[12] Sugar, J., Kaufman, V., and Cooper, D.: 1982, Phys, Scr. (in press).Google Scholar
[13] Edlen, B.: 1982, Phys. Scr. 26, pp. 7183.Google Scholar
[14] Strlganov, A.R. and Odintsova, G.A.: 1982, “Tables of Spectral Lines of Atoms and Ions,” Energolzdat, Moscow, U.S.S.R. Google Scholar
[15] Kelly, R.L.: 1982, “Atomic and Ionic Spectrum Lines Below 2000 Angstroms - Hydrogen through Argon,” to be published.Google Scholar
[16] Moore, C.E.: 1982, Nat. Stand. Ref. Data Ser., Nat. Bur. Stand. (U.S.) 3 Sec. 10 (in press).Google Scholar
[17] Martin, W.C. and Zalubas, R.: 1983, J. Phys. Chem. Ref. Data, to be published.Google Scholar
[18] Kaufman, V.: 1982, Phys. Scr., submitted for publication.Google Scholar
[19] Litzén, U., Physics Department, University of Lund, Sweden, and Brault, J.W., work in progress.Google Scholar
[20] Svendenius, N., Magnusson, C.E., and Zetterberg, P.O., Physics Department, University of Lund, Sweden, to be published.Google Scholar
[21] Jupen, C., et al., Physics Department, University of Lund, Sweden, work in progress.Google Scholar
[22] Engström, L., et al., Physics Department, University of Lund, Sweden, to be published.Google Scholar
[23] Joelsson, I., Zetterberg, P.O., and Magnusson, C.E., Physics Department, University of Lund, Sweden, work in progress.Google Scholar
[24] Johansson, S., Physics Department, University of Lund, Sweden, and Garcia-Riquelme, O., Instituto de Optica, Madrid 6, Spain, et al., work in progress.Google Scholar
[25] Pettersson, J.E., to be submitted to Phys. Scr. Google Scholar
[26] Ekberg, J.O., Physics Department, University of Lund, Sweden, work in progress.Google Scholar
[27] Okasaka, R. and Fukuda, K.: 1982, J. Phys. B 15, pp. 357370.Google Scholar
[28] Connerade, J.P., Baig, M.A., and Newsom, G.H.: 1981, Proc. R. Soc. London, Ser. A 378, pp. 445460.Google Scholar
[29] Learner, R.C.M., Physics Dept. Imperial College of Science and Technology, London SW7, U.K., and Brault, J.W., work in progress.Google Scholar
[30] Brown, C.M. and Ginter, M.L., Naval Research Laboratory, Washington, D.C., 20375, U.S.A., unpublished Fe I absorption data (1530-3214 Å).Google Scholar
[31] Hinnov, E., Suckewer, S., Cohen, S., and Sato, K. : 1982, Phys. Rev. A 25, pp. 22932301. Google Scholar
[32] Baig, M.A., Connerade, J.P., and Newsom, G.H.: 1979, Proc. R. Soc. London, Ser. A 367, pp. 381394.Google Scholar
[33] Johansson, S.: 1978, Phys. Scr. 18, pp. 217265; also see Ref. [114] in the Report.Google Scholar
[34] Ekberg, J.O. and Edlen, B.: 1978, Phys. Scr. 18, pp. 107124.Google Scholar
[35] Pettersson, S.G.: 1982, “The Spectrum of 0 III,” thesis, Dept. of Physics, Lund Institute of Technology, Lund 7, Sweden; Phys. Scr. (in press).Google Scholar
[36] Kaufman, V., and Martin, W.C., unpublished wavelength determinations for the O VI 2s-2p resonance doublet. The values obtained were 1031.926±0.007 Å and 1037.620±0.005 Å.Google Scholar
[37] Iglesias, L.: 1982, Opt. Pura Apl. (in press).Google Scholar
[38] Epstein, G.L. and Reader, J.: 1982, J. Opt. Soc. Am. 72, pp. 476492.CrossRefGoogle Scholar
[39] Meinders, E., Meijer, F.G., and Remijn, L.: 1982, Phys. Scr. 25, pp. 527535.CrossRefGoogle Scholar
[40] van Kleef, T.A.M. and Joshi, Y.N.: 1981, Phys. Scr. 24, pp. 557565.Google Scholar
[41] Wyart, J.F. and Kaufman, V.: 1981, Phys Scr. 24, pp. 941952.CrossRefGoogle Scholar
[42] Corliss, C. and Sugar, J.: 1982, J. Phys. Chem. Ref. Data 11, pp. 135241.Google Scholar
[43] Sugar, J. and Corliss, C.: 1981, J. Phys. Chem. Ref. Data 10, pp. 10971174.Google Scholar
[44] Cheng, K.T., Kim, Y.-K., and Desclaux, J.P.: 1979, At. Data Nucl. Data Tables 24, pp. 111189.Google Scholar
[45] Reader, J., Corliss, C.H., Wlese, W.L., and Martin, G.A.: 1980, “Wavelengths and Transition Probabilities for Atoms and Atomic Ions,” NSRDS-NBS 68, 415 pp. Available from Superintendent of Documents, U.S. Government Printing Office, Washington, D.C. 20402, U.S.A. (Price $14).Google Scholar
[46] Reader, J. and Corliss, C.H., Eds.: 1982, “Line Spectra of the Elements,” in: CRC Handbook of Chemistry and Physics, 63rd Edition, (Weast, R.C., ed.), CRC Press, Boca Raton, FL, U.S.A. Google Scholar
[47] Kelly, R.L.: 1979, “Atomic Emission Lines in the Near Ultraviolet; Hydrogen through Krypton,” NASA Tech. Memorandum 80268, Sec. I (by element, 403 pp.) and Sec. II (by wavelength, 384 pp.) Available from National Technical Information Service, 5285 Port Royal Road, Springfield, VA 22161, U.S.A. Request Sec I, NASA N 80-32190, and Sec. II, NASA N 80-32191.Google Scholar
[48] Fawcett, B.C.: 1981, Phys. Scr. 24, pp. 663680.Google Scholar
[49] Martinson, I.: 1981, Phys. Scr. 23, 126135.CrossRefGoogle Scholar
[50] Cowan, R.D.: 1981, Phys. Scr. 24, pp. 615621.Google Scholar
[51] Feldman, U.: 1981, Phys. Scr. 24, pp. 681711.Google Scholar
[52] Katsonis, K., Ed.: “International Bulletin on Atomic and Molecular Data for Fusion,” Atomic and Molecular Data Unit, Nuclear Data Section, International Atomic Energy Agency, Wagramerstrasse 5, P.O. Box 100, A-1400 Vienna, Austria.Google Scholar
[53] Crandall, D.H., Barnett, C.F., and Wlese, W.L., Eds.: “Atomic Data for Fusion,” Oak Ridge National Laboratory, P.O. Box X., Bldg. 6003, Oak Ridge, TN 37830, U.S.A. Google Scholar
[54] Hansen, J.E. and Persson, W.,: 1982, Phys. Scr. 25, pp. 487490.Google Scholar
[55] Edlen, B.: Proc. 5th General Conf. European Physical Society, in press. (See Ref. [13] also.)Google Scholar
[56] van Kleef, T.A.M., Podobedova, L.I., Ryabtsev, A.N., and Joshi, Y.N.: 1982: Phys. Rev. A 25, pp. 20172030. Google Scholar
[57]Reports on Astrononmy”: 1982, Trans. I.A.U. XVIIIA, pp. 134139.Google Scholar
[58] Brown, C.M.: 1980, Astron. and Ap. 88, pp. 273274. (This reference was included in [57], but keyed only to O V.)Google Scholar