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Communication Dans Un Congrès Année : 2017

Photochemical Escape of Oxygen from Mars: Consequences for Climate History

Résumé

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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insu-01664627 , version 1 (15-12-2017)

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  • HAL Id : insu-01664627 , version 1

Citer

R. Lillis, Justin 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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