Hostname: page-component-6bf8c574d5-9f2xs Total loading time: 0 Render date: 2025-03-09T15:13:32.847Z Has data issue: false hasContentIssue false
  • English
  • Français

Laboratory-Produced Radiation Related to the Solar Flare Emission

Published online by Cambridge University Press:  12 April 2016

R. C. Elton  and
T. N. Lie
R. C. Elton
Affiliation:
U.S. Naval Research Laboratory, Washington, D.C. 20390, U.S.A.
T. N. Lie
Affiliation:
U.S. Naval Research Laboratory, Washington, D.C. 20390, U.S.A.

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.

A review is given of continuing efforts to generate laboratory spectra at photon energies above 1 keV from highly ionized atoms. Emphasis is placed on the most easily-interpreted highest ion stages such as the hydrogenic, helium-like and lithium-like species. The close similarities to solar flare observations of certain signatures, such as the line and continuum X-ray spectra and microwave emission as well as their sequence of occurrence, are pointed out and scaling factors are given.

Type
Section V / The Solar Flare Plasma
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 747 - 760
Copyright
Copyright © Reidel 1972

References

Cline, T. L., Holt, S. S., and Hones, E. W. Jr.: 1968, J. Geophys. Res. Space Phys. 73, 434.Google Scholar
Cohen, L., Feldman, U., Swartz, M., and Underwood, J. H.: 1968, J. Opt. Soc. Am. 58, 843.Google Scholar
Connerade, J. P., Peacock, N. J., and Speer, R. J.: 1970, Solar Phys. 14, 159.Google Scholar
Doschek, G. A., Meekins, J. F., Kreplin, R. W., Chubb, T. A., and Friedman, H.: 1971, Astrophys. J. 170, 1573.CrossRefGoogle Scholar
Edlén, B.: 1947, Physica 13, 545; and other papers referenced here.Google Scholar
Elton, R. C.: 1968, Determination of Electron Temperatures between 50 e V and 100 keV from X-Ray Continuum Radiation in Plasmas, NRL Report 6738.Google Scholar
Flernberg, H.: 1942, Arkiv Mat. Astron. Fysik 28, 1.Google Scholar
House, L. L.: 1969, Astrophys. J. Suppl. 18, 21; also Cowan, R. D. (private communication) for Tixix.Google Scholar
Kane, S. R. and Anderson, K. A.: 1970, Astrophys. J. 162, 1003; See also Kane, S. R., this issue, p. 822.Google Scholar
Lee, J. H., Loebbaka, D. S., and Roos, C. E.: 1971a, Plasma Phys. 13, 347.Google Scholar
Lee, J. H., Shomo, L. P., Williams, M. D., and Hermansdörfer, H.: 1971b, Phys. Fluids 14, 2217.CrossRefGoogle Scholar
Lie, T. N. and Elton, R. C.: 1971, Phys. Rev. A3, 865.Google Scholar
Lie, T. N. and Elton, R. C.: 1972, to be published.Google Scholar
Mather, J. W.: 1971, in Lovberg, R. H. and Griem, H. R. (eds.), Methods of Experimental Physics, -Plasma Physics, Vol. 9B, Chapt. 15, Academic Press, New York.Google Scholar
Neupert, W. M. and Swartz, M.: 1970, Astrophys. J. Letters 160, L189.Google Scholar
Peacock, N. J., Speer, R. J., and Hobby, M. G.: 1969, J. Phys. B. 2, 798.Google Scholar
Peacock, N. J., Hobby, M. G., and Morgan, P. D.: 1971, Proceedings Fourth Conference on Plasma Physics and Controlled Nuclear Fusion Research, Madison, Wisconsin. IAEA, Vienna 1, 537.Google Scholar