Theoretical studies of the faint features in the S0(0) line of H2 observed in the Voyager IRIS mission

Details Theoretical studies of the faint features in the S0(0) line of H2 observed in the Voyager IRIS mission Theoretical studies of the faint features in the S0(0) line of H2 observed in the Voyager IRIS mission

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...182l..40s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 182, no. 2, Aug. 1987, p. L40-L42.

Astronomy and Astrophysics

Astrophysics

12

Absorption Spectra, Astronomical Models, H Lines, Infrared Spectra, Jupiter Atmosphere, Radiant Flux Density, Atomic Spectra, Iris Satellites, Molecular Spectra, Saturn Atmosphere, Voyager Project

Scientific paper

The faint features of the S0(0) line of H2 observed at the Jovian atmosphere in the Voyager IRIS mission have been made subject of thorough theoretical studies. The presently best available non-spherical interaction potential of H2-H2 and very recently improved ab initio results of the induced dipole moment have been used for obtaining absorption spectra which are quantitatively reliable. Some significant corrections of previously published theoretical results have been found and are discussed in this letter.

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