| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701618 | Icarus | 2013 | 11 Pages |
Abstract
⺠IR extinction spectra could contribute to identifying martian cloud properties. ⺠IR spectra of CO2, CO2-H2O, and CO2-dust cloud particles show distinctive features. ⺠Experiments reveal that CO2 forms patches on H2O cores instead of a complete shell.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Merrill Isenor, Rafael Escribano, Thomas C. Preston, Ruth Signorell,