Desaturation of H2 quadrupole lines in the atmospheres of the outer planets

Details Desaturation of H2 quadrupole lines in the atmospheres of the outer planets Desaturation of H2 quadrupole lines in the atmospheres of the outer planets

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...271..859c&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 271, Aug. 15, 1983, p. 859-864.

Astronomy and Astrophysics

Astrophysics

17

Desaturation, Gas Giant Planets, Hydrogen, Molecular Spectra, Planetary Atmospheres, Quadrupoles, Absorption Spectra, Atmospheric Composition, Atmospheric Models, Spectral Line Width, Planets, Giant Planets, Saturation, Hydrogen, Quadrupoles, Atmosphere, Absorption, Abundance, Uranus, Neptune, Models, Spectra

Scientific paper

The vibrational dependence of self-broadening of molecular hydrogen lines results in a desaturation of quadrupole absorption lines long thought to be highly saturated in planetary atmospheres. This desaturation significantly alters H2 abundances in the atmospheres of Uranus and Neptune. The authors present baseline models to illustrate the effects of the revision of this fundamental H2 parameter.

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