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Seasonal changes in the vertical structure of ozone in the Martian lower atmosphere and its relationship to water vapour.

Documentation:
Ozone and water vapour volume mixing ratio vertical profiles in the Martian atmosphere derived from solar occultation mid-infrared spectra recorded by the Atmospheric Chemistry Suite on the ExoMars Trace Gas Orbiter. Data were recorded between mid Mars year 34 to early Mars year 36. Trace gas retrievals were done using the JPL Gas Fitting Software.

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Creator
ORCID:
0000-0002-2173-9889


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Funder identifier:
http://dx.doi.org/10.13039/501100000038
Grant:
PDF–516895–2018
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Funder identifier:
http://dx.doi.org/10.13039/501100008861
Grant:
ST/T002069/1


Publisher:
University of Oxford
Publication date:
2022
Spatial coverage:
Mars
DOI:
Data collected:
2018-04-21 - 2021-08-10


Language:
English
Keywords:
Subjects:
Deposit date:
2022-01-26

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