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Autor Jiménez Díaz, Alberto |
Documentos disponibles escritos por este autor (26)
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Egea-González, Isabel ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Mansilla, Federico ; Holmes, James A. ; Lewis, Stephen R. ; Patel, Manish R. ; Ruiz Pérez, Javier | Elsevier | 2019Elysium Planitia and Oxia Planum are plains located near the Martian dichotomy. Lately, both regions have been extensively analyzed due to the major role that they play in the InSight and ExoMars missions. InSight landed in Elysium Planitia and [...]texto impreso
Jiménez Díaz, Alberto ; Ruiz Pérez, Javier ; Pérez Gussinyé, Marta ; Kirby, John F. ; Álvarez Gómez, José Antonio ; Tejero López, Rosa ; Capote del Villar, Ramón | Elsevier Science B.V., Amsterdam | 2014As a proxy for long-term lithospheric strength, the effective elastic thickness (Te) can be used to understand the relationship between lithospheric rheology and geodynamic evolution of complex tectonic settings. Here we present, for the first t[...]texto impreso
Arenas Martín, Ricardo ; Fernández Suárez, Javier ; Montero, Pilar ; Díez Fernández, Rubén ; Andonaegui Moreno, Pilar ; Sánchez Martínez, Sonia ; Albert Roper, Richard ; Fuenlabrada Pérez, José Manuel ; Matas, Jerónimo ; Martín Parra, Luis Miguel ; Rubio Pascual, Francisco J. ; Jiménez Díaz, Alberto ; Pereira, M. Francisco | Elsevier | 2018-07In the Ossa Morena Domain of SW Iberia, the Calzadilla Ophiolite is formed by an ensemble of ultramafic and mafic rocks that seem to represent a fragment of an oceanic Moho transition zone. The ophiolite consists of a main sheet with a minimum t[...]texto impreso
Arenas Martín, Ricardo ; Díez Fernández, Rubén ; Rubio Pascual, Francisco J. ; Sánchez Martínez, Sonia ; Martín Parra, Luis Miguel ; Matas, J. ; González del Tánago y del Río, José ; Jiménez Díaz, Alberto ; Fuenlabrada Pérez, José Manuel ; Andonaegui Moreno, Pilar ; Garcia Casco, Antonio | Sociedad Geológica de España. | 2016Correlation of a group of allochthonous terranes (referred to as basal, ophiolitic and upper units) exposed in the NW and SW of the Iberian Massif, is used to propose a new geotectonic zone in the southern branch of the Variscan Orogen: the Gali[...]texto impreso
Arenas Martín, Ricardo ; Díez Fernández, Rubén ; Rubio Pascual, Francisco J. ; Sánchez Martínez, Sonia ; Martín Parra, Luis Miguel ; Matas, Jerónimo ; González del Tánago y del Río, José ; Jiménez Díaz, Alberto ; Fuenlabrada, José M. ; Andonaegui Moreno, Pilar ; Garcia Casco, Antonio | Elsevier | 2016-06Correlation of a group of allochthonous terranes (referred to as basal, ophiolitic and upper units) exposed in theNW and SW of the Iberian Massif, is used to propose a new geotectonic zone in the southern branch of theVariscan Orogen: the Galici[...]texto impreso
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Ruiz Pérez, Javier ; McGovern, Patrick ; Jiménez Díaz, Alberto ; López, Valle ; Williams, Jean-Pierre ; Hahn, Brian C. ; Tejero López, Rosa | Elsevier Science B.V., Amsterdam | 2011Lithospheric strength can be used to estimate the heat flow at the time when a given region was deformed, allowing us to constrain the thermal evolution of a planetary body. In this sense, the high (> 300 km) effective elastic thickness of the l[...]texto impreso
Jiménez Díaz, Alberto ; Ruiz Pérez, Javier ; Villaseca González, Carlos ; Tejero López, Rosa ; Capote del Villar, Ramón | Elsevier Science B.V | 2012In this work we have modeled the thermal structure of the lithosphere of the Spanish Central System and the Tajo Basin, and their implications for lithospheric strength. For his, we have used refined heatproducing elements (HPE) values to obtai[...]texto impreso
Jiménez Díaz, Alberto ; Egea González, Isabel ; Parro, Laura M. ; Tasaka, Miki ; Ruiz Pérez, Javier | Elsevier | 2020In depth knowledge of the thermal and rheological properties of the crust and mantle of Mars is fundamental for constraining the strength of its lithosphere, and thereby for the understanding its geodynamics, tectonics, and thermal evolution. In[...]texto impreso
Egea-González, Isabel ; Jiménez Díaz, Alberto ; Parro, Laura M. ; López, Valle ; Williams, Pierre ; Ruiz Pérez, Javier | Elsevier | 2017-05-15The circum-Hellas area of Mars borders Hellas Planitia, a giant impact ?4.0–4.2 Ga old making the deepest and broadest depression on Mars, and is characterized by a complex pattern of fracture sets, lobate scarps, grabens, and volcanic plains. T[...]