Skip to main content
SpringerLink
Log in

Evidence for temporal variations of coronal emission line intensity and profile

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

The time sequence of line profiles of Fe xiv emission obtained at the 1965 solar eclipse is examined for temporal variations of intensity and profile. Although no variations are found in some regions examined, two regions with intensity and profile line width variations are found. A simple temperature wave is consistent with observations.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  • Billings, D. E.: 1959, Astrophys. J. 130, 215.

    Google Scholar 

  • Jordan, C.: 1969, Monthly Notices Roy. Astron. Soc. 142, 501.

    Google Scholar 

  • Leighton, R. B., Noyes, R. W., and Simon, G. W.: 1962, Astrophys. J. 135, 474.

    Google Scholar 

  • Liebenberg, D. H.: 1975, Solar Phys. 44, 331.

    Google Scholar 

  • Liebenberg, D. H. and Hoffman, M. M.: 1974, in G. Newkirk (ed.), ‘Coronal Disturbances’, IAU Symp. 57, 485.

  • Liebenberg, D. H., Bessey, R. J., and Watson, 1975a, Solar Phys. 40, 387.

    Google Scholar 

  • Liebenberg, D. H., Bessey, R. J., and Watson, 1975b, Solar Phys. 44, 345.

    Google Scholar 

  • Lilliequist, C.: 1965, American Astron. Soc. Meeting, October.

  • Noxon, J. F.: 1966, Astrophys. J. 145, 400.

    Google Scholar 

Download references

Author information

Authors and Affiliations

  1. University of California, Los Alamos Scientific Laboratory, 87545, Los Alamos, NM, U.S.A.

    D. H. Liebenberg

  2. University of Wyoming, 82071, Laramie, WY, U.S.A.

    R. J. Bessey

  3. EG&G, 87544, Los Alamos, NM, U.S.A.

    B. Watson

Authors
  1. D. H. Liebenberg
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. R. J. Bessey
    View author publications

    You can also search for this author in PubMed Google Scholar

  3. B. Watson
    View author publications

    You can also search for this author in PubMed Google Scholar

Additional information

Work performed under the auspices of the U.S. Energy Research and Development Administration.

Work accomplished at the Department of Physics and Astronomy, University of Wyoming, Laramie, Wyoming.

Rights and permissions

Reprints and permissions

About this article

Cite this article

Liebenberg, D.H., Bessey, R.J. & Watson, B. Evidence for temporal variations of coronal emission line intensity and profile. Sol Phys 50, 109–112 (1976). https://doi.org/10.1007/BF00206195

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00206195

Keywords

Search

Navigation