Professeure à l'Université de Paris / Institut de Physique du Globe de Paris
Publications
Lucas, A., S. Rodriguez, F. Lemonnier, A. Le Gall, C. Ferrari, P. Paillou, C. Narteau (2019). Texture and composition of Titan’s equatorial region inferred from Cassini SAR inversion: Implications for aeolian transport at Saturn’s largest moon. JGR, under revision.
Tiscarino, M. et al. (2019) Close-range remote sensing of Saturn’s rings during Cassini’s ring grazing orbits and grand finale. Science, 364, Issue 6445, eaau1017
Labarre, S., S. Jacquemoud, C. Ferrari and the Carolina Team (2019). Retrieving soil surface roughness with the Hapke photometric model: Confrontation with the ground truth. Remote Sensing of Environment, 225, 1-15 .
Ferrari, C.(2018) Thermal properties of icy surfaces in the outer solar system. Space Science Rev., 214, 111.
Spilker, L., Ferrari, C., Altobelli, N., Pilorz, S. and Morishima, R. (2018) Thermal properties of rings and ring particles, in “Planetary Ring Systems: Properties, Structure, and Evolution.” Cambridge University Press Planetary Science Series. M. Tiscareno and C. Murray, Eds.
Jennings, D., Flasar, M.F., Kunde, V.G. and the CIRS Team (2017). The Composite infrared spectrometer (CIRS) on Cassini, Applied Optics, 56(18) 5274-5294.
Labarre, S., C. Ferrari, S. Jacquemoud (2017). Surface roughness retrieval by inversion of the Hapke model: a multiscale approach. Icarus, 290,63-80.
Ferrari, C. and A. Lucas (2016). Low thermal Inertia of Icy Planetary Surfaces: Evidence for amorphous ice? A & A, 588, A133.
Reffet, E., Verdier, M., Ferrari, C. (2015). Thickness of Saturn’s B ring as derived from seasonal temperature variations measured by CIRS Cassini. Icarus, 254, 276 – 286.
Spilker, L., Ferrari, C. and Morishima, R.(2013) Saturn’s rings temperature at equinox. Icarus, 226, 316-322.
Ferrari, C., Reffet, E. (2013). The d ark side of Saturn’s B ring: seasons as clues to its structure. Icarus,223, 28–39.
Ferrari, C., Brooks, S., Edgington, S., Leyrat, C., Pilorz, S., Spilker, L. (2009). Structure of self-gravity wakes in Saturn’s A ring as measured by Cassini CIRS. Icarus, 199, 145–154.
Leyrat, C., Ferrari, C., Charnoz, S. Decriem, J., Spilker, L. Pilorz, S., (2008). Spinning particles in Saturn’s C ring from mid-infrared observations: pre-Cassini mission results. Icarus,196, 625-641.
Leyrat, C., Spilker, L.J., Altobelli, N., Pilorz, S., Ferrari, C. (2008). Infrared observations of Saturn’s rings by Cassini CIRS: Phase angle and local time dependence. Planet. Space Sci, 56, 117-133.
Coustenis A., Atreya, SK., Ferrari, C. et al.Special issue on the Surfaces and atmospheres of the outer planets, their satellites and ring systems (2008). Planet.Space.Sci.,56, 1-2.
Spilker, L., Pilorz, S., Wallis, B., Pearl, J. Cuzzi, J., Brooks, S., Altobelli, N., Edgington, S., Showalter, M., Flasar, M., Ferrari, C. and C. Leyrat (2006). Cassini Thermal Observations of Saturn’s Main Rings: Implications for Particle Rotation and Vertical Mixing, Planet. Space Sci.54, 1167-1176.
Coustenis A., Atreya SK., Ferrari, C. et al.Special issue on the Surfaces and atmospheres of the outer planets, their satellites and ring systems (2006) Planet.Space.Sci., 54, 12, 1115-1116.
Ferrari, C. and C. Leyrat (2006) Thermal emission of spinning particles ring particles: the standard model. Astron. Astroph.,447, 745-760.
Flasar F. M., et al. (2005): Titan’s atmospheric temperatures, winds and composition, Science, 308, 975-978
Ferrari C., Galdemard P., Lagage P.O., Pantin, E. and C. Quoirin (2005) Imaging Saturn’s rings with CAMIRAS: Thermal inertia of B and C rings. Astron. Astroph., 441, 379-389.
Coustenis A., Ferrari C., Atreya SK. et al.Special issue on the Surfaces and atmospheres of the outer planets, their satellites and ring systems (2005). Planet.Space.Sci., 53, 5, 459-460.
Flasar F. M. et al. (2005) Temperatures, winds and composition in the Saturnian system. Science, 307,1247-1251
Flasar F. M. et al. (2004) Exploring the Saturn System in the Thermal Infrared: The Composite Infrared Spectrometer, Space Sci. Rev., 115, 169-297.
Flasar F. M. et al. (2004) Exploring the Saturn System in the Thermal Infrared: The Composite Infrared Spectrometer, in the Cassini-Huygens Mission – Orbiter Remote Sensing Investigations, Kluwer academic Publishers.
Kunde, V. G et al. (2004) Jupiter’s Atmospheric Composition from the Cassini Thermal Infrared Spectroscopy Experiment, Science, Science, 305, 1582-1586.
Flasar, F. M., et al. (2004) An intense stratospheric jet on Jupiter, Nature, 427, 132-135.
Ferrari, C (2004)-Saturn’s satellitew and rings: Huygens’ heritage. Ed. Fletcher, K in Proceedings of the International Conference Titan: From Discovery To Encounter Pages: 281-290.
Spilker, L., Ferrari, C., Cuzzi, J., Showalter, M., Pearl, J. and B. Wallis (2003) Saturn’s rings in thermal infrared, in Surfaces and atmospheres of the outer planets, their satellites and ring systems, Review paper, Special issue, Planet.Space.Sci., 51, 929-935.
Coustenis A., Spilker, L., Atreya S., Ferrari C., Surfaces and atmospheres of the outer planets, their satellites and ring systems (2003)- Foreword, Planet.Space.Sci., 51, 14-15.
Charnoz S., Brahic A., Ferrari C., Grenier I., Roddier F., P. Thébault (2001) Detection of arcs in Saturn’s F ring during the Sun’s ring plane crossing in 1995. Astron. Astroph., 365, 214-225.
Rannou P., Ferrari C., Rage K., Roos-Serote M. and M. Cabane (2000), Characterization of aerosols in the detached haze layer of Titan. Icarus, 147, 267-281.
Ferrari, C. and A. Brahic (1997), Arcs and clumps in the Encke Division of Saturn’s Rings. Planet. Space Sci., 45, No. 9, 1051-1067.
Roddier, F. et al. (1996), Satellites of Saturn, Circ. IAU No. 6407.
Ferrari, C. and A. Brahic (1994) Azimuthal Brightness Asymmetries in Planetary Rings: I. Neptune’s Arcs and Narrow Rings, Icarus, 111, 193-210.
Brahic, A. and C. Ferrari (1991), Planetary rings: observational constraints and collision dynamics, IAU Symposium N.152 – Chaos, resonance and collective dynamical Phenomena in the Solar System. Angras dos Rios, Brasil.
Sicardy, B. et al. (1990), Probing the Titan Atmosphere by the July 8, 1989 occultation of 28 Sgr, Nature,343, 25 January 1990.