The albedo, effective temperature, and energy balance of Uranus, as determined from Voyager IRIS data

Author:

Pearl J.C.,Conrath B.J.,Hanel R.A.,Pirraglia J.A.,Coustenis A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference39 articles.

1. Collission induced spectra of the H2He interaction from 79 K to 248 K between 200 and 700 cm−1;Bachet;Bull. Amer. Astron. Soc.,1986

2. The translational-rotational absorption spectrum of hydrogen;Bachet;Canad. J. Phys.,1983

3. A model of the spatial and temporal variations of the Uranus thermal structure;Bezard,1985

4. Theory of the line shape in passive induced absorption;Birnbaum;Canad. J. Phys.,1976

5. Thermal structure of Jupiter's atmosphere obtained by inversion of Voyager 1 infrared measurements;Conrath,1980

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