The most recent analysis of the Voyager ultraviolet solar occultation observations at Neptune indicates a methane mixing ratio 1-10 times above saturation in the lower stratosphere, unlike the value of 500-1000 times saturation which was suggested just before the encounter of Voyager with Neptune. The acetylene mixing ratio in the 0.1 mb region is found to be (6-8) x 10 exp -8, which is approximately a factor of 3 lower than the value reported in our Voyager/Science paper. The eddy diffusion coefficient at the homopause (1-3) x 10 exp 7 sq cm/s, is found to be more like that of Saturn than Uranus. The new results on CH4, C2H2 and K have strong implications for the stratospheric temperatures, now warmer, and the source of heating. Furthermore, the pre-Voyager models of the hydrocarbon hazes need to be revised in view of the new model atmosphere.
Hydrocarbons and eddy mixing in Neptune's atmosphere
Advances in Space Research ; 12 , 11, N
1992-11-01
Sonstige
Keine Angabe
Englisch
Hydrocarbons and eddy mixing in Neptune's atmosphere
Elsevier | 1992
|Vertical Structure of Neptune's Atmosphere
NTRS | 1996
|Online Contents | 2010
|AIAA | 1992
Elsevier | 1992
|