Interesting lines in the infrared solar spectrum. II. Unblended lines between λ1.0 and λ1.8 μm.

Details Interesting lines in the infrared solar spectrum. II. Unblended lines between λ1.0 and λ1.8 μm. Interesting lines in the infrared solar spectrum. II. Unblended lines between λ1.0 and λ1.8 μm.

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26as..113...71r&link_type=abstract

Astronomy and Astrophysics Supplement, v.113, p.71

Astronomy and Astrophysics

Astrophysics

13

Lines: Profiles, Lines: Identification, Atomic Data, Sun: Infrared

Scientific paper

We list 603 spectral lines between 1.0 and 1.8μm that are judged to be relatively unblended from a visual inspection of spectra of the quiet sun. Much of the atomic data of relevance to studies of solar and stellar magnetism, convection and atmospheric structure are also provided. Particular attention is paid to blending by telluric lines. We determine the level of blending both in the presence and the absence of telluric lines. We also describe how telluric blends may be removed from spectra with high spectral resolution.

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