New emission bands in the high resolution spectrum of molecular nitrogen between 107.7 and 124.2nm

Details New emission bands in the high resolution spectrum of molecular nitrogen between 107.7 and 124.2nm New emission bands in the high resolution spectrum of molecular nitrogen between 107.7 and 124.2nm

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39.1301r&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 39, Sept. 1991, p. 1301-1304. Research supported by CNRS.

Physics

9

Emission Spectra, Molecular Gases, Nitrogen, Planetary Atmospheres, Ultraviolet Spectra, Dayglow, Satellite Atmospheres, Spectral Bands, Spectral Resolution, Tables (Data)

Scientific paper

Vacuum ultraviolet (VUV) spectra emitted by planetary atmospheres are analyzed using the Voyager 1 and 2 data, which revealed that the atmospheres of Titan and Triton mainly consist of molecular nitrogen. The VUV emission spectrum of molecular nitrogen is investigated at high spectral resolution from 107.7 to 124.2 nm. Band origins are reported for the 103 bands.

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