| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8138828 | Icarus | 2014 | 10 Pages |
Abstract
The new model has been validated for temperatures up to 313Â K, and may be consistently used for the expected conditions for aqueous clouds in all of the outer planets. The model fits 60.26% of all laboratory measurements within 2-sigma uncertainty. Descriptions of the experimental setups, uncertainties associated with the laboratory measurements, the model fitting process, the new model, and its application to approximating jovian cloud opacity are provided.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Danny Duong, Paul G. Steffes, Sahand Noorizadeh,