Prediction of a CO22+layer in the atmosphere of Mars

Author:

Witasse O.1,Dutuit O.2,Lilensten J.3,Thissen R.2,Zabka J.4,Alcaraz C.5,Blelly P.-L.6,Bougher S. W.7,Engel S.7,Andersen L. H.8,Seiersen K.8

Affiliation:

1. Research and Scientific Support Department of ESA; ESTEC; Noordwijk The Netherlands

2. Laboratoire de Chimie Physique; Centre Universitaire Paris Sud; Orsay France

3. Laboratoire de Planétologie de Grenoble; France

4. V. Cermak Laboratory; Prague Czech Republic

5. Laboratoire LURE; Centre Universitaire Paris Sud; Orsay France

6. Centre d'Etudes Spatiales des Rayonnements; Toulouse France

7. Lunar and Planetary Laboratory; Tucson USA

8. Institute of Physics and Astronomy; Aarhus University; Aarhus Denmark

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference15 articles.

1. Berthelier DYMIX (Dynamics of the Martian Ionosphere and Exosphere) 1997

2. Blelly , P.-L. 8-moment fluid model of the terrestrial high latitude ionosphere between 100 and 3000 km Solar Terrestrial Energy Program: Handbook of ionospheric models 1996

3. Comparative Terrestrial Planet Thermospheres: 2. Solar Cycle Variation of Global Structure and Winds at Equinox;Bougher;J. Geophys. Res.,1999

4. Comparative Terrestrial Planet Thermospheres: 3. Solar Cycle Variation of Global Structure and Winds at Solstices;Bougher;J. Geophys. Res.,2000

5. A numerical model of the ionosphere, including the E-region above EISCAT;Diloy;Annales Geophysicae,1996

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