Published September 3, 2022
| Version v1
Poster
Open
Characterization of the Martian atmosphere: global model comparison with NOMAD data
Authors/Creators
- 1. Instituto de Astrofísica de Andalucía - CSIC
- 2. Laboratoire de Météorologie Dynamique - IPSL
- 3. LATMOS, IPSL
- 4. Open University
- 5. Istituto Nazionale de Astrofisica
- 6. Belgian Institute for Space Aeronomy
Description
Poster for the SEA 2022 meeting describing the comparison between ExoMars NOMAD solar occultation observations retrieved at the Instituto de Astrofísica de Andalucía and the predictions of a ground-to-exobase Global Climate Model. The temperature structure and the abundances of CO2, CO, and H2O in the mesosphere (up to ~100 km) are compared.
Notes
This work was supported by the Spanish Ministry of Science and Innovation, the Agencia Estatal de Investigación, and by the UE FEDER funds under grants RTI2018-100920-J-I00 and PGC2018-101836-BI00. The IAA/CSIC team acknowledges financial support from the State Agency for Research of the Spanish MCIU through the 'Center of Excellence Severo Ochoa' award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709)
Files
gonzalezgalindo_SEA2022_poster.pdf
Files
(108.3 MB)
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