Re-analysis of an observed solar near-infrared eclipse spectrum

Details Re-analysis of an observed solar near-infrared eclipse spectrum Re-analysis of an observed solar near-infrared eclipse spectrum

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..143..197k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 143, no. 1, p. 197-200.

Physics

7

Forbidden Bands, Infrared Spectra, Near Infrared Radiation, Solar Eclipses, Solar Spectra, Spectrum Analysis, Forbidden Transitions, H I Regions, Helium, Hydrogen

Scientific paper

The spectroscopic assignments of Olsen et al. (1971), for their observed solar eclipse wavelengths in the near-IR region between 1 and 3 microns, are reviewed in the light of more recent information. Several assignments are shown to need revision, and alternate candidates are proposed, including the possibility of an interesting forbidden line emitted from the high metastable level 3s3p3d (4F9/2) of Fe XIV.

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