Zobrazeno 1 - 10
of 204
pro vyhledávání: '"Hueso , Ricardo"'
Autor:
Hue, Vincent, Cavalié, Thibault, Sinclair, James A., Zhang, Xi, Benmahi, Bilal, Rodríguez-Ovalle, Pablo, Giles, Rohini S., Stallard, Tom S., Johnson, Rosie E., Dobrijevic, Michel, Fouchet, Thierry, Greathouse, Thomas K., Grodent, Denis C., Hueso, Ricardo, Mousis, Olivier, Nixon, Conor A.
Observations of the Jovian upper atmosphere at high latitudes in the UV, IR and mm/sub-mm all indicate that the chemical distributions and thermal structure are broadly influenced by auroral particle precipitations. Mid-IR and UV observations have sh
Externí odkaz:
http://arxiv.org/abs/2410.20413
Autor:
From, Jorge, Hernández-Bernal, Jorge, Moinelo, Alejandro Cardesin, Hueso, Ricardo, Ravanis, Eleni, Sierra, Abel Burgos, Wood, Simon, Sitja, Marc Costa, Escalante, Alfredo, Grotheer, Emmanuel, de la Parra, Julia Marin Yaseli, Merrit, Donald, Almeida, Miguel, Breitfellner, Michel, Sierra, Mar, Martin, Patrick, Titov, Dmitri, Wilson, Colin, Larsen, Ethan, Gaztelurrutia, Teresa del Rio, Lavega, Agustin Sanchez
The Visual Monitoring Camera (VMC) is a small imaging instrument onboard Mars Express with a field of view of ~40x30 degrees. The camera was initially intended to provide visual confirmation of the separation of the Beagle 2 lander and has similar te
Externí odkaz:
http://arxiv.org/abs/2410.02999
Autor:
Harkett, Jake, Fletcher, Leigh N., King, Oliver R. T., Roman, Michael T., Melin, Henrik, Hammel, Heidi B., Hueso, Ricardo, Sánchez-Lavega, Agustín, Wong, Michael H., Milam, Stefanie N., Orton, Glenn S., de Kleer, Katherine, Irwin, Patrick G. J., de Pater, Imke, Fouchet, Thierry, Rodríguez-Ovalle, Pablo, Fry, Patrick M., Showalter, Mark R.
Publikováno v:
JGR:Planets, 129, e2024JE008415
Jupiter's Great Red Spot (GRS) was mapped by the James Webb Space Telescope (JWST)/Mid-Infrared Instrument (4.9-27.9 micron) in July and August 2022. These observations took place alongside a suite of visual and infrared observations from; Hubble, JW
Externí odkaz:
http://arxiv.org/abs/2410.02468
Publikováno v:
Space Science Reviews (2024) 220:8
Deep elemental composition is a challenging measurement to achieve in the giant planets of the solar system. Yet, knowledge of the deep composition offers important insights in the internal structure of these planets, their evolutionary history and t
Externí odkaz:
http://arxiv.org/abs/2407.07515
Autor:
Rodríguez-Ovalle, Pablo, Fouchet, Thierry, Guerlet, Sandrine, Cavalié, Thibault, Hue, Vincent, López-Puertas, Manuel, Lellouch, Emmanuel, Sinclair, James A., de Pater, Imke, Fletcher, Leigh N., Wong, Michael H., Harkett, Jake, Orton, Glenn S., Hueso, Ricardo, Sánchez-Lavega, Agustín, Stallard, Tom S., Bockelee-Morvan, Dominique, King, Oliver, Roman, Michael T., Melin, Henrik
Jupiters south polar region was observed by JWST Mid Infrared Instrument in December 2022. We used the Medium Resolution Spectrometer mode to provide new information about Jupiters South Polar stratosphere. The southern auroral region was visible and
Externí odkaz:
http://arxiv.org/abs/2406.08133
Autor:
Mousis, Olivier, Cavalié, Thibault, Lunine, Jonathan I., Mandt, Kathleen E., Hueso, Ricardo, Aguichine, Artyom, Schneeberger, Antoine, Couzinou, Tom Benest, Atkinson, David H., Hue, Vincent, Hofstadter, Mark, Srisuchinwong, Udomlerd
The exploration of carbon-to-oxygen ratios has yielded intriguing insights into the composition of close-in giant exoplanets, giving rise to a distinct classification: carbon-rich planets, characterized by a carbon-to-oxygen ratio $\ge$ 1 in their at
Externí odkaz:
http://arxiv.org/abs/2405.19748
Autor:
Hueso, Ricardo, Peralta, Javier, Garate-Lopez, Itziar, Bandos, Tatyana V., Sanchez-Lavega, Agustin
Publikováno v:
Planetary and Space Science, 113-114, 78-99 (2015)
Venus Express provided a long-term monitoring of Venus atmosphere. Several works focused on the dynamics of the upper cloud visible on the day-side in ultraviolet images sensitive to the 65-70 km altitude and in the lower cloud level (50 km height) o
Externí odkaz:
http://arxiv.org/abs/2401.17046
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
Autor:
Chavez, Erandi, de Pater, Imke, Redwing, Erin, Molter, Edward M., Roman, Michael T., Zorzi, Andrea, Alvarez, Carlos, Campbell, Randy, de Kleer, Katherine, Hueso, Ricardo, Wong, Michael H., Lynam, Elinor Gates Paul David, Davies, Ashley G., Aycock, Joel, Mcilroy, Jason, Pelletier, John, Ridenour, Anthony, Stickel, Terry
Publikováno v:
Icarus Volume 404, 1 November 2023, 115667
Using archival near-infrared observations from the Keck and Lick Observatories and the Hubble Space Telescope, we document the evolution of Neptune's cloud activity from 1994 to 2022. We calculate the fraction of Neptune's disk that contained clouds,
Externí odkaz:
http://arxiv.org/abs/2307.08157
Autor:
Chavez, Erandi, Redwing, Erin, de Pater, Imke, Hueso, Ricardo, Molter, Edward M., Wong, Michael H., Alvarez, Carlos, Gates, Elinor, de Kleer, Katherine, Aycock, Joel, Mcilroy, Jason, Pelletier, John, Ridenour, Anthony, Sánchez-Lavega, Agustín, Rojas, Jose Félix, Stickel, Terry
Publikováno v:
Icarus Volume 401, 1 September 2023, Article 115604
Using near-infrared observations of Neptune from the Keck and Lick Observatories, and the Hubble Space Telescope in combination with amateur datasets, we calculated the drift rates of prominent infrared-bright cloud features on Neptune between 2018 a
Externí odkaz:
http://arxiv.org/abs/2307.06462