| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701619 | Icarus | 2013 | 7 Pages |
Abstract
⺠Visible and near infrared O2 emissions on the Venus nightside are modeled. ⺠Differences in peak altitudes are interpreted in terms of collisional deactivation. ⺠We predict higher altitude of the Chamberlain emission than the Herzberg II bands. ⺠We compare with limb observations from VIRTIS onboard Venus Express. ⺠We derive values for yields of O2 molecules and collisional quenching coefficients.
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Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
J.-C. Gérard, L. Soret, A. Migliorini, G. Piccioni,