Photochemical Escape of Oxygen from Mars: Consequences for Climate History

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
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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 : jeudi 11 janvier 2018 - 06:27:17

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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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