Información del autor
Autor Jiménez Díaz, Alberto |
Documentos disponibles escritos por este autor (26)
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Jiménez Díaz, Alberto | 2008-09En este trabajo se estudian los macizos situados en el Anticlinorio de Olivenza-Monesterio, prestando especial atención al macizo Cerro Cabrera. Este cuerpo contiene mineralizaciones de Cr, Ni, Cu y Elementos del Grupo del Platino de característ[...]texto impreso
Torres López, Sara ; Muñoz Martín, Alfonso ; Jiménez Díaz, Alberto ; Ahmed, Baba ; De lorenzo, Javier ; García López, Cristina ; Olaiz Campos, Antonio José | Sociedad Geológica de España | 2010The aim of this study is the hydrogeological exploration and characterization using Geophisical surveying in the vicinity of Dakhla Basin (Algeria). To that end, it has been used the method of resistivities through Vertical Electric Sounding (VE[...]texto impreso
El estudio de la estructura térmica y mecánica de la litosfera aporta información sobre el modo en que las capas externas y relativamente rígidas de los planetas, responden a las fuerzas a las que se encuentran sometidas. También proporciona inf[...]texto impreso
García Mayordomo, Julián ; Insua Arévalo, Juan Miguel ; Martínez Díaz, José J. ; Jiménez Díaz, Alberto ; Martín Banda, Raquel ; Martín Alfageme, Santiago ; Álvarez Gómez, José Antonio ; Rodríguez Peces, Martín Jesús ; Pérez López, Raúl ; Rodríguez Pascua, Miguel Angel ; Masana, E. ; Perea Manea, Hector ; Martín González, Fidel ; Giner Robles, Jorge ; Nemserb, Eliza S. ; Cabral, Joao | Universidad Complutense de Madrid | 2012La Base de Datos de Fallas Activas de Iberia (QAFI) es una iniciativa promovida por el Instituto Geológico y Minero de España (IGME) para construir un repositorio público de información científica sobre fallas con actividad en los últimos 2,59 M[...]texto impreso
Ruiz Pérez, Javier ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Egea González, Isabel ; Mansilla, Federico | Elsevier | 2019-04Two recent papers, by Karimi et al. (2016, Icarus 272, 102–113) and Karimi and Dombard (2017, Icarus 282, 34–39), tried to deduce paleo-heat flows for, respectively, Mars and Venus from modeling the viscoelastic relaxation of large impact crater[...]texto impreso
García Mayordomo, Julián ; Insua Arévalo, Juan Miguel ; Jiménez Díaz, Alberto ; Álvarez Gómez, José Antonio ; Rodríguez Peces, Martín Jesús | 2011Recientemente se han producido en España una serie de iniciativas encaminadas a aprovechar el conocimiento geológico para la definición y la caracterización de fuentes sismogénicas enfocadas al cálculo de la peligrosidad sísmica en Iberia. En es[...]texto impreso
Díez Fernández, Rubén ; Jiménez Díaz, Alberto ; Arenas Martín, Ricardo ; Pereira, M. Francisco ; Fernández Suárez, Javier | American Geophysical Union | 2019-01The Calzadilla Ophiolite is an ensemble of mafic and ultramafic rocks that represents the transition between lower crust and upper mantle of a Cadomian (peri?Gondwanan) fore arc. Mapping and structural analysis of the ophiolite demonstrates that[...]texto impreso
Jiménez Díaz, Alberto ; Ruiz Pérez, Javier ; Tejero López, Rosa ; Kirby, John F. ; Capote del Villar, Ramón | Sociedad Geológica de España. | 2016Como indicador de la resistencia de la litosfera a largo plazo, el espesor elástico efectivo (Te) se puede utilizar para entender la relación entre la reología de la litosfera y la evolución geodinámica de ambientes tectónicos complejos. En este[...]texto impreso
Ruiz Pérez, Javier ; Jiménez Díaz, Alberto ; Parro, Laura M. ; Mansilla, Federico ; Egea González, Isabel ; Küppers, Michael | Nature Research | 2019-07-01The surface of the dwarf planet Ceres is considered to be dominated by geological processes typical of small bodies or medium-sized icy bodies, such as impact cratering; there are also features of putative cryovolcanic origin as well as those re[...]texto impreso
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Jiménez Díaz, Alberto ; Capote del Villar, Ramón ; Tejero López, Rosa ; Lunar Hernández, Rosario ; Ortega Menor, Lorena ; Monterrubio Pérez, Serafín ; Maldonado, Casimiro ; Rodríguez, David | Sociedad Geológica de España | 2009The Los Llanos Shear Zone bounds the Cabeza Gorda and Zafra units located in the Ossa-Morena Zone (SW Iberian Massif). Within the Cabeza Gorda unit two peridotitic massifs crop out, named Sierra Cabeza Gorda and Cerro Cabrera. The mylonitic rock[...]texto impreso
The Valles Marineris canyon system in Mars shows large landslides across its walls, which can be 40 km wide and up to 60 km long, with fall scarps height as high as 7 km. These landslides were produced through a large mass movement at high speed[...]texto impreso
Jiménez Díaz, Alberto ; Egea González, Isabel ; Parro, Laura ; Tasaka, Miki ; Ruiz Pérez, Javier | United States. National Aeronautics and Space Administration | 2017An adequate knowledge of thermal and rheological properties of crust and mantle is fundamental for deciphering and understanding the thermal state and interior evolution of a planetary body. Previously, indirect methods have been used to calcula[...]texto impreso
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Parro, Laura M. ; Jiménez Díaz, Alberto ; Mansilla, Federico ; Ruiz Pérez, Javier | Nature Publishing Group | 2017-04-03Until the acquisition of in-situ measurements, the study of the present-day heat flow of Mars must rely on indirect methods, mainly based on the relation between the thermal state of the lithosphere and its mechanical strength, or on theoretical[...]texto impreso
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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[...]