Zobrazeno 1 - 10
of 90
pro vyhledávání: '"T. del Río‐Gaztelurrutia"'
Autor:
A. Sánchez-Lavega, A. García-Muñoz, T. del Río-Gaztelurrutia, S. Pérez-Hoyos, J. F. Sanz-Requena, R. Hueso, S. Guerlet, J. Peralta
Publikováno v:
Nature Communications, Vol 11, Iss 1, Pp 1-8 (2020)
The authors analyze a system of multi-layered hazes above Saturn’s hexagonal-wave cloud tops in the visual range. Analyses suggest the formation to be caused by condensation processes, and the vertical distribution of stacked layers by the upward p
Externí odkaz:
https://doaj.org/article/7e7e897f8c104839b874a53d89cfb253
Autor:
A. Sánchez-Lavega, E. García-Melendo, S. Pérez-Hoyos, R. Hueso, M. H. Wong, A. Simon, J. F. Sanz-Requena, A. Antuñano, N. Barrado-Izagirre, I. Garate-Lopez, J. F. Rojas, T. del Río-Gaztelurrutia, J. M. Gómez-Forrellad, I. de Pater, L. Li, T. Barry
Publikováno v:
Nature Communications, Vol 7, Iss 1, Pp 1-10 (2016)
The origin, variability, and structure of Saturn’s intense and broad eastward equatorial jet at upper cloud level are complex and unexplained. Here, based on observations of a large, bright equatorial disturbance in 2015, the authors characterise t
Externí odkaz:
https://doaj.org/article/9e37e6d3b86343cab8590fa165dae3dd
Akademický článek
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Autor:
R. Hueso, C. E. Newman, T. del Río‐Gaztelurrutia, A. Munguira, A. Sánchez‐Lavega, D. Toledo, V. Apéstigue, I. Arruego, A. Vicente‐Retortillo, G. Martínez, M. Lemmon, R. Lorenz, M. Richardson, D. Viudez‐Moreiras, M. de la Torre‐Juarez, J. A. Rodríguez‐Manfredi, L. K. Tamppari, N. Murdoch, S. Navarro‐López, J. Gómez‐Elvira, M. Baker, J. Pla‐García, A. M. Harri, M. Hieta, M. Genzer, J. Polkko, I. Jaakonaho, T. Makinen, A. Stott, D. Mimoun, B. Chide, E. Sebastian, D. Banfield, A. Lepinette‐Malvite
We characterize vortex and dust devils (DDs) at Jezero from pressure and winds obtained with the Mars Environmental Dynamics Analyzer (MEDA) instrument on Mars 2020 over 415 Martian days (sols) (Ls = 6°–213°). Vortices are abundant (4.9 per sol w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e077cc691a5077bbd1c999c469e3e552
https://doi.org/10.1002/essoar.10512158.1
https://doi.org/10.1002/essoar.10512158.1
Akademický článek
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Autor:
Jose Rodriguez-Manfredi, Manuel de la Torre Juarez, Agustin Sanchez-Lavega, Ricardo Hueso, German Martinez, Mark Lemmon, Claire Newman, Asier Munguira, Maria Hieta, Leslie Tamppari, Jouni Polkko, Daniel Toledo, Eduardo Sebastian, Michael Smith, Iina Jaakonaho, Maria Genzer, Alvaro de Vicente-Retortillo, Daniel Viudez-Moreiras, Miguel Ramos, Alfonso Saiz-Lopez, Alain Lepinette, Michael Wolff, Robert Sullivan, Javier Gómez-Elvira, Victor Apestigue, Pamela Conrad, T. del Río-Gaztelurrutia, Naomi Murdoch, Ignacio Arruego, Donald Banfield, Justin Boland, Adrian Brown, Joaquin Ceballos, Manuel Dominguez-Pumar, Servando Espejo, Alberto Fairen, Ricardo Ferrandiz, Erik Fischer, Miriam Garcia-Villadangos, Silvia Gimenez, Felipe Gomez-Gomez, Scott Guzewich, Ari-Matti Harri, Juan Jimenez, Vicente Jimenez, Teemu Makinen, Mercedes Marin-Jimenez, Carolina Martin-Rubio, Javier Martin-Soler, Antonio Molina, Luis Mora-Sotomayor, Sara Navarro Lopez, Veronica Peinado, Isabel Perez-Grande, Jorge Pla-Garcia, Marina Postigo, Olga Prieto-Ballesteros, Scot Rafkin, Mark Richardson, Julio Romeral, Catalina Romero, Hannu Savijärvi, John Schofield, Josefina Torres, Roser Urqui, Sofia Zurita, MEDA team
Perseverance's Mars Environmental Dynamics Analyzer (MEDA) is collecting data at Jezero Crater, characterizing the physical processes in the lowest layer of the atmosphere as no previous instrument did before. Here we show that temperature measuremen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dc91d910d7218602b9ffd4f42ca7a730
https://doi.org/10.21203/rs.3.rs-1634885/v1
https://doi.org/10.21203/rs.3.rs-1634885/v1
Autor:
Eleni Ravanis, Alejandro Cardesín-Moinelo, T. del Río-Gaztelurrutia, Agustín Sánchez-Lavega, R. Hueso, Jorge Hernández-Bernal, Dmitri Titov, Simon Wood
Publikováno v:
Geophysical Research Letters. 48
We present the first systematic study of clouds observed during twilight on Mars. We analyze images obtained by the Visual Monitoring Camera (VMC) on Mars Express between 2007 and 2020. Using an automated retrieval algorithm we found 407 cases of clo
Autor:
Kyle Connour, Nicholas M. Schneider, R. Jaumann, T. del Río-Gaztelurrutia, Dmitrij Titov, Eleni Ravanis, Daniela Tirsch, B. Gondet, Alejandro Cardesín-Moinelo, R. Hueso, Ernst Hauber, Agustín Sánchez-Lavega, Simon Wood, I. Ordonez-Etxeberria, Jorge Hernández-Bernal
We report a previously unnoticed annually repeating phenomenon consisting of the daily formation of an extremely elongated cloud extending as far as 1,800 km westward from Arsia Mons. It takes place in the solar longitude (Ls) range of ∼220°-320°
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7f35cf5902f1583cc140bef554a8013
http://arxiv.org/abs/2103.03919
http://arxiv.org/abs/2103.03919
Autor:
Dmitrij Titov, Jorge Hernández-Bernal, A. de Burgos-Sierra, T. del Río-Gaztelurrutia, Agustín Sánchez-Lavega, Alejandro Cardesín-Moinelo, Eleni Ravanis, Simon Wood, R. Hueso
We study the 2018 Martian Global DustStorm (GDS 2018) over the Southern Polar Region using images obtained by the Visual Monitoring Camera (VMC) on board Mars Express during June and July 2018. Dust penetrated into the polar cap region but never cove
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd8df87aa141dfe75008e9613bb0f231
http://arxiv.org/abs/2102.13521
http://arxiv.org/abs/2102.13521
Autor:
K. Ahrens-Velásquez, Manel Soria, M. H. Wong, T. del Río-Gaztelurrutia, Amy Simon, Enrique Garcia-Melendo, T. Barry, C. Foster, R. Hueso, Agustín Sánchez-Lavega, C. Go
Publikováno v:
UPCommons. Portal del coneixement obert de la UPC
Universitat Politècnica de Catalunya (UPC)
Geophysical Research Letters
Universitat Politècnica de Catalunya (UPC)
Geophysical Research Letters
In March 2020 a convective storm erupted at planetographic latitude 76°N in the southern flank of Saturn’s long-lived hexagonal wave. The storm reached a zonal size of 4,500 km and developed a tail extending zonally 33,000 km. Two new short-lived
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b4634d3b29a616ba50655a65bb56b381
http://hdl.handle.net/2117/345836
http://hdl.handle.net/2117/345836