Radiative Transfer Modeling in Titan's Atmosphere and Surface: Application to Cassini/VIMS Data Analysis at Regional to Global Scale - Laboratoire Atmosphères, Milieux, Observations Spatiales Access content directly
Conference Papers Year : 2024

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

Abstract

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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Dates and versions

insu-04545906 , version 1 (14-04-2024)

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  • HAL Id : insu-04545906 , version 1

Cite

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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