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.
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References
Allen, C. W.: 1963,Astrophysical Quantities, Oxford University Press, Inc., New York.
Bely, O. and Faucher, P.: 1969,Astron. Astrophys. 1, 37.
Burgess, A.: 1964,Astrophys. J. 138, 5.
Burgess, A.: 1965,Astrophys. J. 141, 1588.
Griem, H. R.: 1969,Astrophys. J. 156, L103.
House, L. L.: 1969,Astrophys. J. Suppl. 18, No. 155, 21.
Meekins, J. F., Doschek, G. A., Friedman, H., Chubb, T. A., and Kreplin, R. W.: 1970,Solar Phys. 13, 198.
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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
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DOI: https://doi.org/10.1007/BF00963953