| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701748 | Icarus | 2012 | 6 Pages |
Abstract
⺠Extreme UV photodissociation of CO2 generates emissions by the triplet CO states. ⺠CO(a-X) Cameron bands in the Mars dayglow have very high rotational temperatures. ⺠CO rotational excitation and triplet emissions are a diagnostic for CO2 presence.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Konstantinos S. Kalogerakis, Constantin Romanescu, Musahid Ahmed, Kevin R. Wilson, Tom G. Slanger,