Mathieu Hirtzig

Affiliations: 
University Paris 11 
Google:
"Mathieu Hirtzig"

Parents

Sign in to add mentor
Athéna Coustenis grad student 2005 University Paris 11
 (Etude de Titan dans l'infrarouge proche par spectro-imagerie couplée à l'optique adaptative)
BETA: Related publications

Publications

You can help our author matching system! If you notice any publications incorrectly attributed to this author, please sign in and mark matches as correct or incorrect.

Rodriguez S, Le Mouélic S, Barnes JW, et al. (2018) Observational evidence for active dust storms on Titan at equinox Nature Geoscience. 11: 727-732
Brossier JF, Rodriguez S, Cornet T, et al. (2018) Geological Evolution of Titan's Equatorial Regions: Possible Nature and Origin of the Dune Material Journal of Geophysical Research: Planets. 123: 1089-1112
Solomonidou A, Coustenis A, Lopes RMC, et al. (2018) The Spectral Nature of Titan's Major Geomorphological Units: Constraints on Surface Composition Journal of Geophysical Research: Planets. 123: 489-507
Parkinson CD, Gao P, Esposito L, et al. (2015) Photochemical control of the distribution of Venusian water Planetary and Space Science. 113: 226-236
Solomonidou A, Coustenis A, Hirtzig M, et al. (2014) Temporal variations of Titan's surface with Cassini/VIMS Icarus
Solomonidou A, Hirtzig M, Coustenis A, et al. (2014) Surface albedo spectral properties of geologically interesting areas on Titan Journal of Geophysical Research E: Planets. 119: 1729-1747
Solomonidou A, Bampasidis G, Hirtzig M, et al. (2013) Morphotectonic features on Titan and their possible origin Planetary and Space Science. 77: 104-117
Hirtzig M, Bézard B, Lellouch E, et al. (2013) Corrigendum to “Titan’s surface and atmosphere from Cassini/VIMS data with updated methane opacity” [Icarus 226 (2013) 470–486] Icarus. 226: 1182-1182
Hirtzig M, Bézard B, Lellouch E, et al. (2013) Titan's surface and atmosphere from Cassini/VIMS data with updated methane opacity Icarus. 226: 470-486
Bergh Cd, Courtin R, Bézard B, et al. (2012) Applications of a new set of methane line parameters to the modeling of Titan’s spectrum in the 1.58 μm window Planetary and Space Science. 61: 85-98
See more...