Skip to main content
Log in

Recombination edges observed in solar soft X-ray flare spectra

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

Edges in the solar soft X-ray flare continuum have been observed with the NRL Bragg crystal spectrometer aboard OSO-4. The edges near 2.06 Å, 2.8 Å, and 4.46 Å are interpreted to be due to an innershell dielectronic recombination process, details of which are presented. Two other edges, 3.59 Å and 3.31 Å, are interpreted to be due to recombination of the bare sulfur ion and innershell transitions of calcium.

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

Access this article

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

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Allen, C. W.: 1963,Astrophysical Quantities, Oxford University Press, Inc., New York.

    Google Scholar 

  • Bely, O. and Faucher, P.: 1969,Astron. Astrophys. 1, 37.

    Google Scholar 

  • Burgess, A.: 1964,Astrophys. J. 138, 5.

    Google Scholar 

  • Burgess, A.: 1965,Astrophys. J. 141, 1588.

    Google Scholar 

  • Griem, H. R.: 1969,Astrophys. J. 156, L103.

    Google Scholar 

  • House, L. L.: 1969,Astrophys. J. Suppl. 18, No. 155, 21.

    Google Scholar 

  • Meekins, J. F., Doschek, G. A., Friedman, H., Chubb, T. A., and Kreplin, R. W.: 1970,Solar Phys. 13, 198.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Meekins, J.F., Doschek, G.A. Recombination edges observed in solar soft X-ray flare spectra. Sol Phys 13, 213–219 (1970). https://doi.org/10.1007/BF00963953

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00963953

Keywords

Navigation