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
https://hal-insu.archives-ouvertes.fr/insu-01664627
Contributor : Catherine Cardon
<>
Submitted on : Friday, December 15, 2017 - 9:21:36 AM
Last modification on : Wednesday, May 22, 2019 - 4:48:10 PM
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⟩
