Zobrazeno 1 - 10
of 1 614
pro vyhledávání: '"P. Rannou"'
Autor:
M. Es-sayeh, S. Rodriguez, M. Coutelier, P. Rannou, B. Bézard, L. Maltagliati, T. Cornet, B. Grieger, E. Karkoschka, S. Le Mouélic, A. Le Gall, C. Neish, S. MacKenzie, A. Solomonidou, C. Sotin, A. Coustenis
Publikováno v:
The Planetary Science Journal, Vol 4, Iss 3, p 44 (2023)
We present an analysis of Titan data acquired by the Cassini Visual and Infrared Mapping Spectrometer (VIMS) at the landing site of the Dragonfly mission, using a new version of our radiative transfer model for Titan, with significant updates for the
Externí odkaz:
https://doaj.org/article/4b1f068376ee44098b117b659fbe2c81
Publikováno v:
Atmospheric Measurement Techniques, Vol 9, Iss 2, Pp 455-467 (2016)
A small and sophisticated optical depth sensor (ODS) has been designed to work in the atmosphere of Mars. The instrument measures alternatively the diffuse radiation from the sky and the attenuated direct radiation from the Sun on the surface. The pr
Externí odkaz:
https://doaj.org/article/bcf71ea389894f24bef7a0ec2d1acada
Autor:
Mousis, O., Bouquet, A., Langevin, Y., André, N., Boithias, H., Durry, G., Faye, F., Hartogh, P., Helbert, J., Iess, L., Kempf, S., Masters, A., Postberg, F., Renard, J. -B., Vernazza, P., Vorburger, A., Wurz, P., Atkinson, D. H., Barabash, S., Berthomier, M., Brucato, J., Cable, M., Carter, J., Cazaux, S., Coustenis, A., Danger, G., Dehant, V., Fornaro, T., Garnier, P., Gautier, T., Groussin, O., Hadid, L. Z., Ize, J. -C., Kolmasova, I., Lebreton, J. -P., Maistre, S. Le, Lellouch, E., Lunine, J. I., Mandt, K. E., Martins, Z., Mimoun, D., Nenon, Q., Caro, G. M. Munõz, Rannou, P., Rauer, H., Schmitt-Kopplin, P., Schneeberger, A., Simons, M., Stephan, K., Van Hoolst, T., Vaverka, J., Wieser, M., Wörner, L.
Enceladus, an icy moon of Saturn, possesses an internal water ocean and jets expelling ocean material into space. Cassini investigations indicated that the subsurface ocean could be a habitable environment having a complex interaction with the rocky
Externí odkaz:
http://arxiv.org/abs/2211.00721
Autor:
Rodriguez, Sébastien, Vinatier, Sandrine, Cordier, Daniel, Tobie, Gabriel, Achterberg, Richard K., Anderson, Carrie M., Badman, Sarah V., Barnes, Jason W., Barth, Erika L., Bézard, Bruno, Carrasco, Nathalie, Charnay, Benjamin, Clark, Roger N., Coll, Patrice, Cornet, Thomas, Coustenis, Athena, Couturier-Tamburelli, Isabelle, Dobrijevic, Michel, Flasar, F. Michael, de Kok, Remco, Freissinet, Caroline, Galand, Marina, Gautier, Thomas, Geppert, Wolf D., Griffith, Caitlin A., Gudipati, Murthy S., Hadid, Lina Z., Hayes, Alexander G., Hendrix, Amanda R., Jauman, Ralf, Jennings, Donald E., Jolly, Antoine, Kalousova, Klara, Koskinen, Tommi T., Lavvas, Panayotis, Lebonnois, Sébastien, Lebreton, Jean-Pierre, Gall, Alice Le, Lellouch, Emmanuel, Mouélic, Stéphane Le, Lopes, Rosaly M. C., Lora, Juan M., Lorenz, Ralph D., Lucas, Antoine, MacKenzie, Shannon, Malaska, Michael J., Mandt, Kathleen, Mastrogiuseppe, Marco, Newman, Claire E., Nixon, Conor A., Radebaugh, Jani, Rafkin, Scot C., Rannou, Pascal, Sciamma-O-Brien, Ella M., Soderblom, Jason M., Solomonidou, Anezina, Sotin, Christophe, Stephan, Katrin, Strobel, Darrell, Szopa, Cyril, Teanby, Nicholas A., Turtle, Elizabeth P., Vuitton, Véronique, West, Robert A.
In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest moon Titan. Titan, a "world with two oceans", is an organic-rich body w
Externí odkaz:
http://arxiv.org/abs/2110.10466
Autor:
Coutelier, Maélie, Cordier, Daniel, Seignovert, Benoît, Rannou, Pascal, Gall, Alice Le, Cours, Thibaud, Maltagliati, Luca, Rodriguez, Sébastien
Titan's surface was revealed by Cassini's instruments, showing the presence of liquid hydrocarbons in lakes, and features like dry riverbed. In order to study the sediment transport in Titan's channels and to map distribution of the water-ice signatu
Externí odkaz:
http://arxiv.org/abs/2104.12719
Publikováno v:
ApJ 907 36 (2021)
This study presents a 13 years survey of haze UV extinction profiles, monitoring the temporal evolution of the detached haze layer (DHL) in Titan's upper atmosphere (350-600 km). As reported by West et al. 2011 (GRL vol.38, L06204) at the equator, we
Externí odkaz:
http://arxiv.org/abs/2102.05384
Stream graphs model highly dynamic networks in which nodes and/or links arrive and/or leave over time. Strongly connected components in stream graphs were defined recently, but no algorithm was provided to compute them. We present here several soluti
Externí odkaz:
http://arxiv.org/abs/2011.08054
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.