Conference papers
Study of the cold oxygen corona with IUVS/MAVEN
Abstract : The Mars Atmosphere and Volatile Evolution Mission (MAVEN) has observed the Martian upper atmosphere for several months. The Imaging Ultraviolet Spectrograph (IUVS) is able to measure the resonance line of the atomic oxygen at 130.4 nm. From this emission we are able to derive information of the oxygen content in the Martian upper atmosphere and its variability. Atomic oxygen is a key species to better understand the chemistry, heating, dynamics and escape of the Martian upper atmosphere.
Cited literature [5 references]
https://hal-insu.archives-ouvertes.fr/insu-01211135
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Tuesday, October 6, 2015 - 2:22:35 PM
Last modification on : Tuesday, November 16, 2021 - 4:48:32 AM
Long-term archiving on: : Thursday, January 7, 2016 - 10:14:41 AM
Contributor : Catherine Cardon Connect in order to contact the contributor
Submitted on : Tuesday, October 6, 2015 - 2:22:35 PM
Last modification on : Tuesday, November 16, 2021 - 4:48:32 AM
Long-term archiving on: : Thursday, January 7, 2016 - 10:14:41 AM
File
EPSC2015-148.pdf
Publisher files allowed on an open archive