Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Isabel Egea González"'
Publikováno v:
Icarus. 322:221-226
Two 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 craters
Publikováno v:
Icarus. 319:367-380
Martian lobate scarps are prominent tectonic structures interpreted to be the topographic expression of large thrust faults generated under compression. Here, we present a structural modeling performed on three large lobate scarps (Ogygis Rupes, Bosp
Autor:
Pablo Moreno García, María Teresa Costado Dios, Isabel Egea González, Francisco F. López-Ruiz, A. Morales-Garoffolo
Publikováno v:
Brazilian Journal of Development. 5:6936-6945
La actividad realizada por el alumnado durante las sesiones practicas de cualquier asignatura es una parte fundamental del proceso de ensenanza-aprendizaje. Estos entornosson ideales para aplicar tecnicas de aprendizaje colaborativo destinadas a que
Autor:
Isabel Egea-González, Paula C. Lois, Alberto Jiménez-Díaz, Ali M. Bramson, Michael M. Sori, Juan-Ángel Tendero-Ventanas, Javier Ruiz
Publikováno v:
Icarus. 383:115073
Autor:
Isabel Egea-González, Paula C. Lois, Alberto Jiménez-Díaz, Michael M. Sori, Ali M. Bramson, Javier Ruiz
The presence of a liquid deposit of water below the South Polar Layered Deposits (SPLD) Region has been reported based on analysis of MARSIS radar data in the Planum Australe area (Orosei et al., 2018). These radar data show bright subsurface reflect
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8601ad4c942ef2fe31dc435c3b678087
https://doi.org/10.5194/epsc2020-841
https://doi.org/10.5194/epsc2020-841
Autor:
Javier Ruiz, James Holmes, Laura M. Parro, Stephen R. Lewis, Alberto Jiménez-Díaz, Isabel Egea-González, Federico Mansilla, Manish R. Patel
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Icarus Volume 353, 1 January 2021, 113379
RODIN. Repositorio de Objetos de Docencia e Investigación de la Universidad de Cádiz
RODIN: Repositorio de Objetos de Docencia e Investigación de la Universidad de Cádiz
Universidad de Cádiz
instname
Icarus Volume 353, 1 January 2021, 113379
RODIN. Repositorio de Objetos de Docencia e Investigación de la Universidad de Cádiz
RODIN: Repositorio de Objetos de Docencia e Investigación de la Universidad de Cádiz
Universidad de Cádiz
Elysium 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 will
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8f7f77c9e642a8d69d92c1c5eea874ed
http://hdl.handle.net/10261/189519
http://hdl.handle.net/10261/189519
Autor:
Isabel Egea-González, Alberto Jiménez-Díaz, Michael Küppers, Laura M. Parro, Javier Ruiz, Federico Mansilla
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
The 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 cratering1,2; there are also features of putative cryovolcanic origin3 as well as those rel
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec961c6b0fe5591a460f14167a2133da
http://hdl.handle.net/10261/186365
http://hdl.handle.net/10261/186365
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
In 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 this
Autor:
Valle López, Isabel Egea-González, Jean-Pierre Williams, Javier Ruiz, Laura M. Parro, Alberto Jiménez-Díaz
Publikováno v:
Icarus
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
The 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. Th
Autor:
Isabel Egea-González, Javier Ruiz
Publikováno v:
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Universidad Complutense de Madrid
E-Prints Complutense. Archivo Institucional de la UCM
instname
Mercury is covered by a megaregolith layer, which constitutes a poor thermally conducting layer that must have an influence on the thermal state and evolution of the planet, although most thermal modeling or heat flow studies have overlooked it. In t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2ce47e14c4e5c2b0563b2c7d74ad2272