Emission lines are classified belonging to 2s 2 2p n -2s2p n+1 transition arrays in the ions Ti XVII, V XVII to XX, Mn XVIII, MN XIX, Fe XIX and Fe XX. The source of these ions is the plasma produced at metallic surfaces irradiated with a neodymium laser beam with a focused power density in the range of 10 12 to 10 13 W cm -2 at the target surface. The data reported can be applied to the interpretation of solar flare spectra.
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Fawcett et al. (1974) studied this question.
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