2018
DOI: 10.1016/j.icarus.2018.06.018
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PFS/MEX limb observations of 4.3-µm CO2 non-LTE emission in the atmosphere of Mars

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Cited by 4 publications
(1 citation statement)
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“…To name a few examples within our own Solar system, in Earth's atmosphere, non-LTE effects are present with visible effects in the form of airglow emissions, as noted for vibrationally excited OH in Charters, Macdonald & Polanyi ( 1971 ), for which level populations have been measured (Noll et al 2020 ). In the atmosphere of Mars, CO 2 has a non-LTE emission feature at 4.3 μm (L ópez- Valverde et al 2005 ;Giuranna et al 2018 ). In the atmosphere of Venus non-LTE emissions have been detected in limb observations for CO (Gilli et al 2015 ) and CO 2 (Gilli et al 2009 ).…”
Section: Discussionmentioning
confidence: 99%
“…To name a few examples within our own Solar system, in Earth's atmosphere, non-LTE effects are present with visible effects in the form of airglow emissions, as noted for vibrationally excited OH in Charters, Macdonald & Polanyi ( 1971 ), for which level populations have been measured (Noll et al 2020 ). In the atmosphere of Mars, CO 2 has a non-LTE emission feature at 4.3 μm (L ópez- Valverde et al 2005 ;Giuranna et al 2018 ). In the atmosphere of Venus non-LTE emissions have been detected in limb observations for CO (Gilli et al 2015 ) and CO 2 (Gilli et al 2009 ).…”
Section: Discussionmentioning
confidence: 99%