Observed spectra due to N = 3 to 4 transitions in Fe XVII and isoelectronic spectra

Details Observed spectra due to N = 3 to 4 transitions in Fe XVII and isoelectronic spectra Observed spectra due to N = 3 to 4 transitions in Fe XVII and isoelectronic spectra

Jan 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.186..113f&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 186, Jan. 1979, p. 113-116.

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Astronomical Spectroscopy, Electron Transitions, Isoelectronic Sequence, Laser Plasmas, Plasma Spectra, Spectrum Analysis, Iron, Metal Ions, Solar Spectra

Scientific paper

An analysis of spectrograms of laser-produced plasmas is extended to include the strongest emission lines due to transitions between levels of principal quantum numbers n = 3 and 4 for ions in the Ne I isoelectronic sequence between K X and Fe XVII. Spectral-line classifications are supported by theoretical Hartree-XR and Slater-Condon computations of wavelengths and oscillator strengths as well as isoelectronic comparisons.

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