Identification of new solar OH lines in the 10-12 micron region

Details Identification of new solar OH lines in the 10-12 micron region Identification of new solar OH lines in the 10-12 micron region

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981apj...248l.133g&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 248, Sept. 15, 1981, p. L133-L135. NASA-NSF-supported research.

Astronomy and Astrophysics

Astrophysics

18

Hydroxyl Emission, Infrared Spectra, Line Spectra, Solar Spectra, Balloon-Borne Instruments, High Resolution, Infrared Interferometers, Molecular Spectra

Scientific paper

High-resolution (0.02/cm) infrared solar spectra obtained with a balloon-borne interferometer reveal new solar absorption features, which appear as regularly spaced quartets, in the 825-960/cm region. The lines are interpreted as high N-double-prime (25-33) pure rotation lines of solar OH. An effective amount of approximately 8 x 10 to the 15th molecules/sq cm of OH is estimated from the spectra.

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