International audienceThe 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
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceObservation of the Martian hot oxygen corona is an important but difficult mea...
International audienceThe Mars Atmosphere and Volatile Evolution Mission (MAVEN) has observed the Ma...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
First observations of the OI 130.4nm resonant line performed by the Imaging Ultraviolet Spectrograph...
International audienceFirst observations of the O I 130.4 nm resonant line performed by the Imaging ...
International audienceFirst observations of the O I 130.4 nm resonant line performed by the Imaging ...
International audienceObservation of the Martian hot oxygen corona is an important but difficult mea...
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceObservation of the Martian hot oxygen corona is an important but difficult mea...
International audienceThe Mars Atmosphere and Volatile Evolution Mission (MAVEN) has observed the Ma...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe Mars Atmosphere and Volatile Evolution mission (MAVEN) has been recently i...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
International audienceThe observations of the O I 130.4 nm resonant line performed by the Imaging Ul...
First observations of the OI 130.4nm resonant line performed by the Imaging Ultraviolet Spectrograph...
International audienceFirst observations of the O I 130.4 nm resonant line performed by the Imaging ...
International audienceFirst observations of the O I 130.4 nm resonant line performed by the Imaging ...
International audienceObservation of the Martian hot oxygen corona is an important but difficult mea...
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceThe Imaging Ultraviolet Spectrograph (IUVS) aboard the Mars Atmosphere and Vol...
International audienceObservation of the Martian hot oxygen corona is an important but difficult mea...