Hydrocarbons in Neptune's stratosphere from Voyager infrared observations

Author:

Bézard Bruno,Romani Paul N.,Conrath Barney J.,Maguire William C.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Reference39 articles.

1. Radiative-convective equilibrium models of Uranus and Neptune;Appleby;Icarus,1986

2. Collision-induced spectra for H2-He interactions from 79 to 248 K between 200 and 700 cm−1;Bachet;J. Quant. Spectrosc. Radiat. Transfer,1988

3. Theory of line shape in pressureinduced absorption;Birnbaum;J. Can. Phys.,1976

4. Hydrocarbon abundances in the Neptune stratosphere from the Voyager UVS ingress solar occultation;Bishop;Bull. Am. Astron. Soc.,1990

5. Ultraviolet spectrometer observations of Neptune and Triton;Broadfoot;Science,1989

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