On the inclusion of the hydrogen dimer in the analysis of Voyager IRIS spectra

Details On the inclusion of the hydrogen dimer in the analysis of Voyager IRIS spectra On the inclusion of the hydrogen dimer in the analysis of Voyager IRIS spectra

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...394l..29c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 394, no. 1, July 20, 1992, p. L29-L32. Research supported by NASA

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Absorption Spectra, Dimers, Hydrogen, Jupiter Atmosphere, Spectrum Analysis, Voyager Project, Computational Astrophysics, Far Infrared Radiation, Para Hydrogen, Radiative Transfer

Scientific paper

Empirical formulas are fitted to existing theoretical absorption spectra of H2-H2 pairs in the far-infrared allowing the inclusion of dimer absorption, parameterized with the height dependence of the para-hydrogen profile, in the calculations. Comparison between synthetic and Voyager IRIS spectra shows that once the dimer absorption is included it is now possible to reproduce the hydrogen portion of the IRIS spectrum to within the precision of the measurements.

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