Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-13T06:26:39.113Z Has data issue: false hasContentIssue false
  • English
  • Français

Analysis of Very High Excitation Fe I Lines (4f–5g) in the Solar Infrared Spectrum

Published online by Cambridge University Press:  03 August 2017

S. Johansson ,
G. Nave ,
M. Geller ,
A. J. Sauval  and
N. Grevesse
S. Johansson
Affiliation:
Department of Physics, University of Lund, Sölvegatan, 14, S-223 62 Lund, Sweden
G. Nave
Affiliation:
Blackett Laboratory, Imperial College of Science, Technology and Medicine, London SW7 2BZ, England
M. Geller
Affiliation:
Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, U.S.A.
A. J. Sauval
Affiliation:
Observatoire Royal de Belgique, avenue circulaire, 3, B-1180 Brussels, Belgium
N. Grevesse
Affiliation:
Institut d'Astrophysique, Université de Liège, B-4000 Cointe-Liège, Belgium

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present a detailed analysis of very high excitation lines (4f–5g) of Fe I which are present in the spectral region 2545–2585 cm–1 in high resolution spectra both in the laboratory and in the ATMOS solar spectra obtained from space. A value of the solar abundance of iron which agrees with the meteoritic value is derived.

Keywords

infrared: starsline: identificationSun: abundances
Type
Part 6: The Infrared Spectrum
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 543 - 548
Copyright
Copyright © Kluwer 1994 

References

Anders, E., and Grevesse, N.: 1989, Geochim. Cosmochim. Acta 53, 197.CrossRefGoogle Scholar
Biémont, E., Brault, J.W., Delbouille, L., Roland, G.: 1985, Astron. Astrophys. Suppl. 61, 107.Google Scholar
Biémont, E. Baudoux, M., Kurucz, R.L., Ansbacher, W., and Prinnington, E.H.: 1991, Astron. Astrophys. 249, 539.Google Scholar
Blackwell, D.E., Booth, A.J., and Petford, A.D.: 1984, Astron. Astrophys. 132, 236.Google Scholar
Carlsson, M., Rutten, R.J., and Shchukina, N.G.: 1992, Astron. Astrophys. 253, 567.Google Scholar
Chang, E.S., and Schoenfeld, W.G.: 1991, Astrophys. J. 383, 450.Google Scholar
Cowley, C.R.: 1971, The Observatory 91, 139.Google Scholar
Farmer, C.B., and Norton, R.H.: 1989, A High-Resolution Atlas of the Infrared Spectrum of the Sun and the Earth Atmosphere from Space, Vol. I: The Sun, NASA Ref. Pub. 1224, Washington, D.C. Google Scholar
Freudenstein, S.A., and Cooper, J.: 1978, Astrophys. J. 224, 1079.Google Scholar
Hannaford, P., Lowe, R.M., Grevesse, N., and Noels, A.: 1992, Astron. Astrophys. (in press).Google Scholar
Holweger, H., Heise, C., and Kock, M.: 1990, Astron. Astrophys. 232, 510.Google Scholar
Holweger, H., Bard, A., Kock, A., and Kock, M.: 1991, Astron. Astrophys. 249, 545.Google Scholar
Johansson, S., and Learner, R.C.M.: 1990, Astrophys. J. 354, 755.Google Scholar
Johansson, S., Nave, G., Learner, R.C.M., and Thorne, A.P.: 1991, in Jaschek, C. and Andrillat, Y. (eds.), The Infrared Spectral Region of Stars, Cambridge Univ. Press, Cambridge, p. 189.Google Scholar
Johansson, S., Nave, G., Geller, M., Sauval, A.J., Grevesse, N., Schoenfeld, W.G., Chang, E.S., and Farmer, C.B.: 1992 (in preparation).Google Scholar
Litzén, U., and Vergès, J.: 1976, Phys. Scripta 13, 240.Google Scholar
Nave, G., Learner, R.C.M., Murray, J.E., Thorne, A.P., and Brault, J.W.: 1992, J. Physique II France 2, 913.Google Scholar
Ridgway, S.T., Carbon, D.F., Hall, D.N.B., and Jewell, J.: 1984, Astrophys. J. Suppl. 54, 177.Google Scholar
Schoenfeld, W.G., Chang, E.S., and Geller, M.: 1993, these proceedings.Google Scholar
Unsöld, A.: 1955, Physik der Sternatmosphären, 2nd ed., Springer-Verlag, Berlin, p. 331.CrossRefGoogle Scholar