Depósito Digital de Documentos de la UAB Encontrados 2 registros  La búsqueda tardó 0.01 segundos. 
1.
12 p, 3.1 MB North polar trough formation due to in-situ erosion as a source of young ice in mid-latitudinal mantles on Mars / Rodriguez, J. Alexis P. (Planetary Science Institute) ; Tanaka, Kenneth L. (Planetary Science Institute) ; Bramson, Ali M. (Purdue University) ; Leonard, Gregory J. (University of Arizona) ; Baker, Victor R. (University of Arizona) ; Zarroca Bonet, Mario (Universitat Autònoma de Barcelona. Departament de Geologia)
The clockwise spiral of troughs marking the Martian north polar plateau forms one of the planet's youngest megastructures. One popular hypothesis posits that the spiral pattern resulted as troughs underwent poleward migration. [...]
2021 - 10.1038/s41598-021-83329-3
Scientific reports, Vol. 11 (March 2021) , art. 6750  
2.
8 p, 2.1 MB Tsunami waves extensively resurfaced the shorelines of an early Martian ocean / Rodriguez, J. Alexis P. (NASA Ames Research Center) ; Fairén, Alberto G. (Cornell University. Department of Astronomy) ; Tanaka, Kenneth L. (United States Geological Survey) ; Zarroca Bonet, Mario (Universitat Autònoma de Barcelona. Departament de Geologia) ; Linares, Rogelio (Universitat Autònoma de Barcelona. Departament de Geologia) ; Platz, Thomas (Freie Universität Berlin. Planetary Sciences and Remote Sensing) ; Komatsu, Goro (Università d'Annunzio. International Research School of Planetary Sciences) ; Miyamoto, Hideaki (University of Tokyo. The University Museum) ; Kargel, Jeffrey S. (University of Arizona. Department of Hydrology & Water Resources) ; Yan, Jianguo (Wuhan University. State Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing) ; Gulick, Virginia C (SETI Institute) ; Higuchi, Kana (Centro de Astrobiología (Madrid)) ; Baker, Victor R. (University of Arizona. Department of Hydrology & Water Resources) ; Glines, Natalie (SETI Institute)
It has been proposed that ~3. 4 billion years ago an ocean fed by enormous catastrophic floods covered most of the Martian northern lowlands. However, a persistent problem with this hypothesis is the lack of definitive paleoshoreline features. [...]
2016 - 10.1038/srep25106
Scientific reports, Vol. 6 (May 2016) , art. 25106  

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