Radiative Transfer Modeling in Titan's Atmosphere and Surface: Application to Cassini/VIMS Data Analysis at Regional to Global Scale - INSU - Institut national des sciences de l'Univers Accéder directement au contenu
Communication Dans Un Congrès Année : 2024

Radiative Transfer Modeling in Titan's Atmosphere and Surface: Application to Cassini/VIMS Data Analysis at Regional to Global Scale

Résumé

We aim at developing an accurate and fast radiative transfer model and inversion scheme for Titan in order to massively invert the Titan VIMS dataset and determine the main chemical species present on Titan’s surface and follow the atmospheric extinction evolution over time.
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insu-04545906 , version 1 (14-04-2024)

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  • HAL Id : insu-04545906 , version 1

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Maël Es-sayeh, S Rodriguez, C Ntinos, L Maltagliati, T Cornet, et al.. Radiative Transfer Modeling in Titan's Atmosphere and Surface: Application to Cassini/VIMS Data Analysis at Regional to Global Scale. 55th Lunar and Planetary Science Conference (LPSC), Mar 2024, The Woodlands, United States. ⟨insu-04545906⟩
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