Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation on Huygens atmospheric and surface measurements and application to the analysis of the VIMS/Cassini observations of the Dragonfly landing area

M Es-Sayeh (1) , S Rodriguez (1) , Maélie Coutelier (2) , Pascal Rannou (3) , B Bézard (4) , L Maltagliati , Thomas Cornet (5) , B Grieger (6) , Erich Karkoschka (7) , Benoît Seignovert (8) , S Le Mouélic (9) , C Sotin (9) , A Coustenis (4)

1 IPG Paris - Institut de Physique du Globe de Paris
2 PLANETO - LATMOS
3 GSMA - Groupe de spectrométrie moléculaire et atmosphérique
4 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics
5 ESAC - European Space Astronomy Centre
6 Aurora Technology BV
7 LPL - Lunar and Planetary Laboratory [Tucson]
8 LGL-TPE - Laboratoire de Géologie de Lyon - Terre, Planètes, Environnement
9 LPG - Laboratoire de Planétologie et Géosciences [UMR_C 6112]

Domaines: Planète et Univers [physics]

M Es-Sayeh, S Rodriguez, Maélie Coutelier, Pascal Rannou, B Bézard, et al.. Updated radiative transfer model for Titan in the near-infrared wavelength range: Validation on Huygens atmospheric and surface measurements and application to the analysis of the VIMS/Cassini observations of the Dragonfly landing area. 16th Europlanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-657. ⟨insu-04545153⟩