Identification on chromium lines in the infrared solar spectrum based on new interferometric measurements

Details Identification on chromium lines in the infrared solar spectrum based on new interferometric measurements Identification on chromium lines in the infrared solar spectrum based on new interferometric measurements

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26as...61..185b&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 61, Aug. 1985, p. 185-190.

Astronomy and Astrophysics

Astrophysics

12

Chromium, Infrared Spectra, Interferometry, Solar Spectra, High Resolution, Oscillator Strengths, Spectral Line Width

Scientific paper

High resolution spectra of chromium obtained by the interferometric method show the presence of several hundreds of new lines in the infrared region (1800 < V < 9000 cm-1). These spectra have been used in order to proceed to the identification of many weak lines on the high resolution solar spectra obtained recently by Delbouille et al. (1981).

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