| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705190 | Planetary and Space Science | 2012 | 9 Pages |
Abstract
⺠Reduction of the mean difference between the model and observations from a factor of 5 to a factor of 3. ⺠Detailed oxygen chemistry on Titan using the full selfconsistent model for Titan's atmosphere and ionosphere. ⺠The model H2O profile is between the CIRS and Herschel H2O observations at 100-250 km and within uncertainties of the ISO and INMS observations. ⺠Huge diversity between upper atmospheres of Triton and Pluto. ⺠Meteorite H2O results in precipitation of CO on Triton and CO2 on Pluto.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
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Authors
Vladimir A. Krasnopolsky,