Photochemical Escape of Oxygen from Mars: Consequences for Climate History

R. Lillis 1 J. Deighan 2 J. L. Fox 3 S. Bougher 4 Y. Lee 4 M. Combi 4 François Leblanc 5 T. Cravens 6 A. Rahmati 6 H. Gröller 7 B. Jakosky 2
1 SSL - Space Sciences Laboratory [Berkeley]
2 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
3 Department of Physics [Dayton]
4 AOSS - Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor]
5 HEPPI - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
6 Department of Physics and Astronomy [Lawrence]
7 Lunar and Planetary Laboratory [Tucson]
Abstract : As well as this effort using in situ data, MAVEN can also constrain photochemical escape using remote sensing of the oxygen corona with the Imaging Ultraviolet Spectrograph (IUVS) [12, 13], the Solar Energetic Particle (SEP) instrument and the Solar Wind Ion Analyzer [14]. These multiple methods will eventually allow validation of photochemical escape from Mars and its dependence on solar and planetary conditions, enabling confident extrapolation back into the past
Type de document :
Communication dans un congrès
Fourth International Conference on Early Mars: Geologic, Hydrologic, and Climatic Evolution and the Implications for Life, Oct 2017, Flagstaff, Arizona, United States. pp.LPI Contribution No. 2014
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https://hal-insu.archives-ouvertes.fr/insu-01664627
Contributeur : Catherine Cardon <>
Soumis le : vendredi 15 décembre 2017 - 09:21:36
Dernière modification le : mercredi 21 mars 2018 - 18:58:12

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R. Lillis, J. Deighan, J. L. Fox, S. Bougher, Y. Lee, et al.. Photochemical Escape of Oxygen from Mars: Consequences for Climate History. Fourth International Conference on Early Mars: Geologic, Hydrologic, and Climatic Evolution and the Implications for Life, Oct 2017, Flagstaff, Arizona, United States. pp.LPI Contribution No. 2014. 〈insu-01664627〉

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