Matches in SemOpenAlex for { <https://semopenalex.org/work/W2069373083> ?p ?o ?g. }
- W2069373083 endingPage "n/a" @default.
- W2069373083 startingPage "n/a" @default.
- W2069373083 abstract "[1] We use a three-dimensional atmospheric model to study the airglow emissions from molecular oxygen in the Martian atmosphere. We estimate the O2 Herzberg I & II, the Chamberlain, and the Infrared Atmospheric band emissions from different sets of kinetic parameters available in the literature. As expected, the enhanced production of atomic oxygen during daytime leads to stronger emissions at 12 hour local time than at 00 hour local time. Nevertheless, at night, the strongest emissions are found in the subtropics and around the terminator where the photochemistry of atomic oxygen is more active. Among the simulated emissions, we find that the Infrared Atmospheric emission is the most intense, as expected, and has maximum intensity reaching a few megarayleighs over the poles during the equinoctial seasons, and an average intensity over the equatorial latitudes of 50 kilorayleighs. We investigate the impact of different levels of water and dust content on airglow and we observe that the airglow structure is modulated by variations in the background atmospheric conditions. Moreover, comparisons of the emission with observations from instruments on board Mars orbiters and with ground-based measurements from Earth allow us to validate the consistency of our airglow model. Finally, we observe that the emission profiles from all band systems show structures; a double-layer profile is very frequent, and is representative of the vertical distribution of the current measurements of O2 nightglow. This paper emphasizes the advantage of using three-dimensional global circulation models for the diagnostic of O2 photochemistry in CO2-dominated atmospheres." @default.
- W2069373083 created "2016-06-24" @default.
- W2069373083 creator A5019293871 @default.
- W2069373083 creator A5039910506 @default.
- W2069373083 creator A5044291296 @default.
- W2069373083 creator A5060854639 @default.
- W2069373083 creator A5066487260 @default.
- W2069373083 date "2012-06-01" @default.
- W2069373083 modified "2023-10-18" @default.
- W2069373083 title "Modeled O<sub>2</sub>airglow distributions in the Martian atmosphere" @default.
- W2069373083 cites W1548365182 @default.
- W2069373083 cites W1639166197 @default.
- W2069373083 cites W1795327620 @default.
- W2069373083 cites W1964798513 @default.
- W2069373083 cites W1965079399 @default.
- W2069373083 cites W1968532895 @default.
- W2069373083 cites W1974401024 @default.
- W2069373083 cites W1976629540 @default.
- W2069373083 cites W1977827704 @default.
- W2069373083 cites W1977918576 @default.
- W2069373083 cites W1980177607 @default.
- W2069373083 cites W1980326891 @default.
- W2069373083 cites W1980968381 @default.
- W2069373083 cites W1982224268 @default.
- W2069373083 cites W1983079246 @default.
- W2069373083 cites W1984265457 @default.
- W2069373083 cites W1984745609 @default.
- W2069373083 cites W1984764581 @default.
- W2069373083 cites W1990475160 @default.
- W2069373083 cites W1996474156 @default.
- W2069373083 cites W1997382902 @default.
- W2069373083 cites W1999314180 @default.
- W2069373083 cites W2001779508 @default.
- W2069373083 cites W2001914015 @default.
- W2069373083 cites W2002051782 @default.
- W2069373083 cites W2002633601 @default.
- W2069373083 cites W2005360045 @default.
- W2069373083 cites W2010910065 @default.
- W2069373083 cites W2012488995 @default.
- W2069373083 cites W2016086698 @default.
- W2069373083 cites W2017022398 @default.
- W2069373083 cites W2017101072 @default.
- W2069373083 cites W2022520061 @default.
- W2069373083 cites W2024368191 @default.
- W2069373083 cites W2028633943 @default.
- W2069373083 cites W2029126734 @default.
- W2069373083 cites W2035094598 @default.
- W2069373083 cites W2035937580 @default.
- W2069373083 cites W2036141595 @default.
- W2069373083 cites W2036648310 @default.
- W2069373083 cites W2050253096 @default.
- W2069373083 cites W2050428743 @default.
- W2069373083 cites W2051889381 @default.
- W2069373083 cites W2053165754 @default.
- W2069373083 cites W2054105967 @default.
- W2069373083 cites W2056787479 @default.
- W2069373083 cites W2057504342 @default.
- W2069373083 cites W2062744509 @default.
- W2069373083 cites W2066875283 @default.
- W2069373083 cites W2069395215 @default.
- W2069373083 cites W2069520530 @default.
- W2069373083 cites W2071007092 @default.
- W2069373083 cites W2075257589 @default.
- W2069373083 cites W2075578824 @default.
- W2069373083 cites W2077583657 @default.
- W2069373083 cites W2077979576 @default.
- W2069373083 cites W2078391654 @default.
- W2069373083 cites W2079247013 @default.
- W2069373083 cites W2079305447 @default.
- W2069373083 cites W2085076608 @default.
- W2069373083 cites W2086614332 @default.
- W2069373083 cites W2087094903 @default.
- W2069373083 cites W2091167360 @default.
- W2069373083 cites W2093278953 @default.
- W2069373083 cites W2093324160 @default.
- W2069373083 cites W2095121620 @default.
- W2069373083 cites W2095336399 @default.
- W2069373083 cites W2095464069 @default.
- W2069373083 cites W2108664387 @default.
- W2069373083 cites W2136969878 @default.
- W2069373083 cites W2142748598 @default.
- W2069373083 cites W2144204469 @default.
- W2069373083 cites W2160202036 @default.
- W2069373083 cites W2161915283 @default.
- W2069373083 cites W2167987251 @default.
- W2069373083 cites W2317160733 @default.
- W2069373083 cites W4240588771 @default.
- W2069373083 doi "https://doi.org/10.1029/2011je003901" @default.
- W2069373083 hasPublicationYear "2012" @default.
- W2069373083 type Work @default.
- W2069373083 sameAs 2069373083 @default.
- W2069373083 citedByCount "7" @default.
- W2069373083 countsByYear W20693730832012 @default.
- W2069373083 countsByYear W20693730832013 @default.
- W2069373083 countsByYear W20693730832017 @default.
- W2069373083 countsByYear W20693730832018 @default.
- W2069373083 countsByYear W20693730832019 @default.
- W2069373083 countsByYear W20693730832020 @default.