Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...47..145b&link_type=abstract
Astronomy and Astrophysics Supplement Series, vol. 47, Jan. 1982, p. 145-157.
Astronomy and Astrophysics
Astrophysics
2
Diatomic Molecules, Infrared Spectra, Molecular Spectra, Solar Spectra, Spectrum Analysis, Sunspots, Tables (Data), Cyanides, Emission Spectra, Near Infrared Radiation, Photosphere, Titanium Oxides
Scientific paper
The present publication of results between 7600-8100 Å represents the fourth part of an analysis of molecular lines in the spectrum of a sunspot. It is an extension of results already published covering 6100-6600, 6600-7100 and 7100-7600 Å. According to this investigation, equivalent widths of molecular lines become increasingly difficult to measure beyond 8030 Å. As no valuable quantitative information is to be expected from the study of the near infrared part of our spectrograms, the analysis stops at 8100 Å.
Boyer Robert
Harvey Jack W.
Sotirovski P.
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