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Mapping the mesospheric CO2 clouds on Mars

Abstract : This climatology of martian clouds will enable us to better characterise the mesospheric structure and dynamics, as very specific conditions (especially low temperatures and a source of condensation nuclei) are required for CO2 ice condensation.
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Submitted on : Wednesday, March 1, 2017 - 10:17:33 PM
Last modification on : Tuesday, November 16, 2021 - 5:19:19 AM
Long-term archiving on: : Tuesday, May 30, 2017 - 6:43:25 PM


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  • HAL Id : insu-01480934, version 1


Albert Leboucher, Anni Määttänen, Joachim Audouard, Brigitte Gondet, Franck Montmessin. Mapping the mesospheric CO2 clouds on Mars . Sixth International Workshop on the Mars Atmosphere: Modelling and Observations, Jan 2017, Granada, Spain. ⟨insu-01480934⟩



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