Identifications of Fe XVII and NI XIX in solar flares based on isoelectronic extrapolations

Details Identifications of Fe XVII and NI XIX in solar flares based on isoelectronic extrapolations Identifications of Fe XVII and NI XIX in solar flares based on isoelectronic extrapolations

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.208p...1j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 208, May 1, 1984, p. 1P-5P. Research supported by the N

Astronomy and Astrophysics

Astronomy

42

Iron, Nickel, Solar Flares, Solar Spectra, Atomic Energy Levels, Electron Transitions, Extrapolation, Isoelectronic Sequence, Line Spectra, Magnetic Dipoles

Scientific paper

Twenty-four lines in solar flare spectra in the region 200 - 410 Å have been identified as transitions between the 2s22p53s, 3p and 3d configurations in Fe XVII and Ni XIX. The identifications are based on isoelectronic extrapolations of differences between experimental and theoretical wavenumbers along the neon-like sequence. A predicted wavelength for the magnetic dipole transition 2s22p5 (3P1 - 3P0) in Fe XVII is also given.

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