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Expected intensities of solar forbidden lines emitted from 2p k (k = 2, 3, 4) configurations

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Abstract

Predicted intensities of all significant transitions within the ground configurations of six-, seven-, and eight-electron ions are tabulated for solar conditions, on a common scale. Some applications of the table entries to line identification and emission measure analysis are presented, including proposed Mg vi classifications for the coronal lines 3488.5 Å and 3502.5 Å.

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Author notes

  1. S. O. Kastner

    Present address: Department of Physics, University of British Columbia, Vancouver, B.C., Canada

Authors and Affiliations

  1. Laboratory for Astronomy and Solar Physics, NASA-Goddard Space Flight Center, 20771, Greenbelt, MD, U.S.A.

    S. O. Kastner

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  1. S. O. Kastner
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Kastner, S.O. Expected intensities of solar forbidden lines emitted from 2p k (k = 2, 3, 4) configurations. Sol Phys 85, 41–51 (1983). https://doi.org/10.1007/BF00148256

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  • DOI: https://doi.org/10.1007/BF00148256

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