Solar line identifications in the calcium isoelectronic sequence

Details Solar line identifications in the calcium isoelectronic sequence Solar line identifications in the calcium isoelectronic sequence

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994soph..151...41k&link_type=abstract

Solar Physics, vol. 151, no. 1, p. 41-49

Physics

1

Abundance, Atomic Structure, Calcium, Isoelectronic Sequence, Line Spectra, Solar Spectra, Spectrum Analysis, Stellar Composition, Chromium, Chromosphere, Identifying, Iron, Manganese, Negative Ions, Nickel, Solar Corona, Titanium

Scientific paper

Wavelength coincidences are noted between laboratory and solar spectral line lists for the twenty-electron ions Ca I, Ti III, Cr V, Mn VI, Fe VII and Ni IX, which imply likely identifications for a large number of unidentified lines in the solar lists. These identifications should be useful, e.g., for improving chromospheric/coronal abundance estimates of the less abundant elements titanium, chromium, and manganese.

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