Three-dimensional modeling of ozone on Mars

By F. Lefévre, S. Lebonnois, F. Montmessin, Francois Forget. 2004

220 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Global and Planetary Change

View Paper: https://www.semanticscholar.org/paper/143896a37bbad4f8b5fba36a9a28293ed4774afd

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Francois Forget
2. R. Wordsworth
3. Ehouarn Millour
4. A. Spiga
5. Jean-Baptiste Madeleine
6. Michael D. Smith
7. F. Montmessin
8. James W. Head III

In Atmospheric Science

1. Francois Forget
2. Michael D. Smith
3. Ehouarn Millour
4. R. Wordsworth
5. J. Chaufray
6. François Leblanc
7. Jean-Baptiste Madeleine
8. Jean-Loup Bertaux

In Global and Planetary Change

1. Michael D. Smith
2. Francois Forget
3. Ehouarn Millour
4. Jean-Baptiste Madeleine
5. R. Haberle
6. J. Murphy
7. J. Leconte
8. R. Wordsworth

Citations in the corpus

• 3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds. (2012, methodology): “This scenario was later challenged when Kasting (1991) published his reanalysis of the Pollack et al. (1987) greenhouse calculations.”
• Amazonian northern mid-latitude glaciation on Mars: A proposed climate scenario (2009, background): “…the propagation of gravity waves, the dust cycle (Newman et al., 2002), the water cycle (Montmessin et al., 2004), the role of the regolith (Böttger et al., 2005), the thermosphere (Coll et al., 2005), the ozone photochemistry (Lefèvre et al., 2004), and the HDO cycle (Montmessin et al., 2005).”
• A new model to simulate the Martian mesoscale and microscale atmospheric circulation: Validation and first results (2009, background): “, 2004], and the photochemical cycles [Lefèvre et al., 2004].”
• Global climate modeling of the Martian water cycle with improved microphysics and radiatively active water ice clouds (2013, methodology): “Therefore, we used the photochemistry module implemented in the GCM [ Lefèvre et al. , 2004] to study the supersaturation of water vapor in dedicated simulations.”
• Origin and role of water ice clouds in the Martian water cycle as inferred from a general circulation model (2004, background): “Kahn [1990] advocated clouds as part of a process leading to an enhanced sequestration of water in the regolith.”
• SPICAM on Mars Express: Observing modes and overview of UV spectrometer data and scientific results (2006, background): “dimensional model distribution of ozone of Lefèvre et al. [2004]. Detailed comments are given by Perrier et al.”
• NOMAD, an Integrated Suite of Three Spectrometers for the ExoMars Trace Gas Mission: Technical Description, Science Objectives and Expected Performance (2018, methodology): “The destruction of ozone is strongly controlled by odd hydrogen radicals (Garcia Munoz et al. 2005; Lefèvre et al. 2004).”
• The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter (2018, methodology): “D) models developed in our team (Forget et al. 1999; Lefèvre et al. 2004; Hartogh et al. 2005).”
• Mars Global Ionosphere‐Thermosphere Model: Solar cycle, seasonal, and diurnal variations of the Mars upper atmosphere (2015, background): “…was originally extended up to about 80 km of altitude [Forget et al., 1999], including all the relevant processes in the lower atmosphere, such as a realistic CO2 condensation scheme, a water cycle [Montmessin et al., 2004], and a photochemical model of the lower atmosphere [Lefèvre et al., 2004].”