Zobrazeno 1 - 10
of 174
pro vyhledávání: '"Lora, Juan M."'
Using an idealised climate model incorporating seasonal forcing, we investigate the impact of rotation rate on the abundance of clouds on an Earth-like aquaplanet, and the resulting impacts upon albedo and seasonality. We show that the cloud distribu
Externí odkaz:
http://arxiv.org/abs/2402.04900
Autor:
Chatain, Audrey, Rafkin, Scot C. R., Soto, Alejandro, Moisan, Enora, Lora, Juan M., Gall, Alice Le, Hueso, Ricardo, Spiga, Aymeric
Publikováno v:
Icarus 411 (2024) 115925
Titan, the largest moon of Saturn, has many lakes on its surface, formed mainly of liquid methane. Like water lakes on Earth, these methane lakes on Titan likely profoundly affect the local climate. Previous studies (Rafkin and Soto 2020, Chatain et
Externí odkaz:
http://arxiv.org/abs/2309.07042
We investigate the characteristics of equatorial waves associated with the maintenance of superrotation in the stratosphere of a Titan general circulation model. A variety of equatorial waves are present in the model atmosphere, including equatorial
Externí odkaz:
http://arxiv.org/abs/2307.06745
Autor:
Lora, Juan M.
Publikováno v:
In Icarus 1 November 2024 422
Publikováno v:
In Icarus 1 January 2025 425
Autor:
Battalio, J. Michael1 (AUTHOR) michael@battalio.com, Lora, Juan M.1 (AUTHOR)
Publikováno v:
Journal of Climate. Jun2024, Vol. 37 Issue 12, p3283-3304. 22p.
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:
Chatain, Audrey, Rafkin, Scot C.R., Soto, Alejandro, Moisan, Enora, Lora, Juan M., Le Gall, Alice, Hueso, Ricardo, Spiga, Aymeric
Publikováno v:
In Icarus 15 March 2024 411
Autor:
Battalio, J. Michael, Lora, Juan M.
Annular modes explain much of the internal variability of Earth's atmosphere but have never been identified on other planets. Using reanalyses for Mars and a simulation for Titan, we demonstrate that annular modes are prominent in the atmospheres of
Externí odkaz:
http://arxiv.org/abs/2102.10463
Autor:
MacKenzie, Shannon M., Birch, Samuel P. D., Horst, Sarah, Sotin, Christophe, Barth, Erika, Lora, Juan M., Trainer, Melissa G., Corlies, Paul, Malaska, Michael J., Sciamma-O'Brien, Ella, Thelen, Alexander E., Turtle, Elizabeth P., Radebaugh, Jani, Hanley, Jennifer, Solomonidou, Anezina, Newman, Claire, Regoli, Leonardo, Rodriguez, Sebastien, Seignovert, Benoit, Hayes, Alexander G., Journaux, Baptiste, Steckloff, Jordan, Nna-Mvondo, Delphine, Cornet, Thomas, Palmer, Maureen, Lopes, Rosaly M. C., Vinatier, Sandrine, Lorenz, Ralph, Nixon, Conor, Czaplinski, Ellen, Barnes, Jason W., Sittler, Ed, Coates, Andrew
Thanks to the Cassini-Huygens mission, Titan, the pale orange dot of Pioneer and Voyager encounters has been revealed to be a dynamic, hydrologically-shaped, organic-rich ocean world offering unparalleled opportunities to explore prebiotic chemistry.
Externí odkaz:
http://arxiv.org/abs/2102.08472