Revised ab initio models for H2 H2 collision-induced absorption at low temperatures

Details Revised ab initio models for H2 H2 collision-induced absorption at low temperatures Revised ab initio models for H2 H2 collision-induced absorption at low temperatures

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007icar..189..544o&link_type=abstract

Icarus, Volume 189, Issue 2, p. 544-549.

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

A revised ab initio calculation of the H2 H2 collision-induced absorption results in significant differences compared with the work of J. Borysow et al. [Borysow, J., Trafton, L., Frommhold, L., Birnbaum, G., 1985. Astrophys. J. 296, 644 654] for wavenumbers greater than 600 cm-1 and temperatures below 120 K. The revision has significant influence on the spectra of Uranus and Neptune, and essentially removes the need for models with “super-solar” helium abundances or stratospheric hazes to explain the spectrum of Uranus.

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