Vertical Aerosol Distribution and Mesospheric Clouds From ExoMars UVIS

The vertical opacity structure of the martian atmosphere is important for understanding the distribution of ice (water and carbon dioxide) and dust. We present a new data set of extinction opacity profiles from the NOMAD/UVIS spectrometer aboard the ExoMars Trace Gas Orbiter, covering one and a half...

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Detalles Bibliográficos
Autores principales: Streeter, Paul M., Sellers, Graham, Wolff, Michael J., Mason, Jonathon P., Patel, Manish R., Lewis, Stephen R., Holmes, James A., Daerden, Frank, Thomas, Ian R., Ristic, Bojan, Willame, Yannick, Depiesse, Cédric, Vandaele, Ann Carine, Bellucci, Giancarlo, López‐Moreno, José Juan
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2022
Materias:
Research Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286791/
https://www.ncbi.nlm.nih.gov/pubmed/35865506
http://dx.doi.org/10.1029/2021JE007065

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9286791/
https://www.ncbi.nlm.nih.gov/pubmed/35865506
http://dx.doi.org/10.1029/2021JE007065

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