Conference papers
Photochemical Escape of Oxygen from Mars: Consequences for Climate History
R. Lillis
1
Justin 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
Y. Lee 4
Author
M. Combi 4
Author
François Leblanc 5
Author IdHAL : francois-leblanc69 ORCID : https://orcid.org/0000-0002-5548-3519
T. Cravens 6
Author
1
SSL - Space Sciences Laboratory [Berkeley] (7 Gauss Way, Berkeley, CA 94720 - United States)
- University of California [Berkeley] (Berkeley, CA - United States)
- University of California (United States)
2
LASP - Laboratory for Atmospheric and Space Physics [Boulder] (1234 Innovation Drive, Boulder, CO 80303-7814 - United States)
- University of Colorado [Boulder] (Boulder, Colorado 80309 - United States)
3
Department of Physics [Dayton] (College of Science and Mathematics, 248 Fawcett Hall - United States)
- Wright State University (3640 Colonel Glenn Hwy, Dayton, Ohio, OH 45435 - United States)
4
AOSS - Department of Atmospheric, Oceanic, and Space Sciences [Ann Arbor] (Ann Arbor, MI 48109 - United States)
- University of Michigan [Ann Arbor] (500 Church Street Ann Arbor, MI 48109-1090 - United States)
- University of Michigan System (Michigan - United States)
5
HELIOS - LATMOS (France)
- LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales (11 boulevard d'Alembert
Quartier des Garennes
78280 - Guyancourt - France)
- UVSQ - Université de Versailles Saint-Quentin-en-Yvelines : UMR8190 (55 avenue de Paris - 78035 Versailles cedex - France)
- UPMC - Université Pierre et Marie Curie - Paris 6 : UMR8190 (4 place Jussieu - 75005 Paris - France)
- INSU - CNRS - Institut national des sciences de l'Univers : UMR8190 (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CNRS - Centre National de la Recherche Scientifique : UMR8190 (France)
6
Department of Physics and Astronomy [Lawrence Kansas] (1082 Malott,1251 Wescoe Hall Dr., Lawrence, KS 66045-758 - United States)
- KU - University of Kansas [Lawrence] (1450 Jayhawk Blvd, Lawrence, KS 66045 - United States)
7
LPL - Lunar and Planetary Laboratory [Tucson] (Tucson, AZ 85721-0092 - United States)
- University of Arizona (Tucson AZ 85721 USA - United States)
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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Conference papers
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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, April 14, 2021 - 3:39:42 AM
Contributor : Catherine Cardon <>
Submitted on : Friday, December 15, 2017 - 9:21:36 AM
Last modification on : Wednesday, April 14, 2021 - 3:39:42 AM
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3023.pdf
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- HAL Id : insu-01664627, version 1
Collections
INSU | CNRS | LATMOS | UPMC | UVSQ | SORBONNE-UNIVERSITE | SU-SCIENCES | SU-TI | GS-ENGINEERING
Citation
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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