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Ruiz Pérez, Javier ; Williams, Jean-Pierre ; Dohm, James M. ; Fernández, Carlos ; López, Valle | Rosen Pub. Group | 2009Heat flow calculations based on geological and/or geophysical indicators can help to constrain the thickness, and potentially the geochemical stratification, of the martian crust. Here we analyze the Warrego rise region, part of the ancient moun[...]texto impreso
Ruiz Pérez, Javier ; Fernández, Carlos ; Gómez Ortiz, David ; Dohm, James M. ; López, Valle ; Tejero López, Rosa | Elsevier Science B.V., Amsterdam | 2008Surface heat flow calculations for the Amenthes region of Mars can be independently performed using the depth to the brittle–ductile transition and the effective elastic thickness of the lithosphere estimated for the Late Noachian/Early Hesperia[...]texto impreso
López, Valle ; Ruiz Pérez, Javier ; Vázquez Hoehne, Antonio | Elsevier Science B.V., Amsterdam | 2015The surface of Mercury shows abundant compressive tectonic landforms, including lobate scarps, wrinkle ridges and high-relief ridges, which are different manifestations of thrust faults, and long-wavelength topography variations, which could be [...]texto impreso
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Ruiz Pérez, Javier ; Williams, Jean-Pierre ; Dohm, James M. ; Fernández, Carlos ; López, Valle | Elsevier Science B.V., Amsterdam | 2013Heat flow is a very important parameter for constraining the thermal evolution of a planetary body. Several procedures for calculating heat flows for Mars from geophysical or geological proxies have been used, which are valid for the time when t[...]texto impreso
Ruiz Pérez, Javier ; López, Valle ; Egea González, Isabel | Elsevier Science B.V., Amsterdam | 2013-07Estimates of lithospheric strength for Mercury, based on the depth of thrust faults associated with large lobate scarps (which were most probably formed previously to similar to 3 Ga) or on the effective elastic thickness of the lithosphere supp[...]texto impreso
Ruiz Pérez, Javier ; Tejero López, Rosa ; Gómez Ortiz, David ; López, Valle | Nova Science Publishers | 2006The existence of features indicative of shorelines of ancient oceans on Mars has been proposed for several authors. In this chapter we revise the topography of possible Martian paleoshorelines, and their consequences for the amount of water infi[...]texto impreso
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Ruiz Pérez, Javier ; López, Valle | 2010texto impreso
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Ruiz Pérez, Javier ; López, Valle ; Dohm, James M. ; Fernández, Carlos | Elsevier Science B.V., Amsterdam | 2012Lobate scarps, thought to be the surface expression of large thrust faults, are the most spectacular contractional tectonic features visible on Mercury. Most lobate scarps follow a general and relatively simple pattern, with a roughly arcuate or[...]texto impreso
Anguita, Francisco ; Farelo, Agustín-Felipe ; López, Valle ; Mas, Cristina ; Muñoz Espadas, María Jesús ; Márquez González, Álvaro ; Ruiz Pérez, Javier | American Geophysical Union | 2001-04-25A photogeoIogical reconnaissance of Viking mosaics and images ofthe Tharsis dome has been carried out. Fifteen new areas of transcurrent faulting have been located which, together with other structures previously detected, support a model in whi[...]texto impreso
Ruiz Pérez, Javier ; Montoya, Lilia ; López, Valle ; Amils Samalot, Ricardo Ignacio | Mary Ann Liebert, Inc. | 2006Europa’s chaos and lenticulae may have been originated in relation to thermal diapirs linked to convective upwellings. Thermal convection and diapirism starts if the ice shell is thicker than a critical value (with details depending on the domin[...]texto impreso
