Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Alberto Jiménez-Díaz"'
Autor:
Alberto Jiménez‐Díaz, Ana M. Negredo, Jon F. Kirby, Pilar Sánchez‐Pastor, Javier Fullea, Javier Ruiz, Marta Pérez‐Gussinyé, Chuanhai Yu
Publikováno v:
Geochemistry, Geophysics, Geosystems, Vol 24, Iss 3, Pp n/a-n/a (2023)
Abstract The Eastern Central Atlantic (ECA) region includes the Azores, Canary, Cape Verde, Great Meteor, and Madeira hotspots. These hotspots exhibit a large variety of characteristics and are rooted in the lithosphere ranging in age from newly crea
Externí odkaz:
https://doaj.org/article/f55c8b0c18e04b099a68f03e409e6809
Autor:
Federico Mansilla, Elena Santos, Javier Ruiz, Alberto Jiménez-Díaz, Juan Luis Arsuaga, Isabel Egea-Gonzalez
Publikováno v:
Ichnos. 29:205-217
Publikováno v:
Geophysical Journal International. 229:487-504
SUMMARY The effective elastic thickness (Te) can reflect lateral change of rheological properties from subducting plate to overlying plate, and aid in understanding the relationship between geodynamic evolution and regional tectonic response to accum
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
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
Autor:
Daniel García-Castellanos, Marc Viaplana-Muzas, Lucía Struth, Laura Rodríguez-Rodríguez, Jaume Vergés, Alberto Jiménez-Díaz
Publikováno v:
Scopus
RUO. Repositorio Institucional de la Universidad de Oviedo
instname
BSGF-Earth Sciences Bulletin, Vol 192, p 45 (2021)
Digital.CSIC. Repositorio Institucional del CSIC
RUO. Repositorio Institucional de la Universidad de Oviedo
instname
BSGF-Earth Sciences Bulletin, Vol 192, p 45 (2021)
Digital.CSIC. Repositorio Institucional del CSIC
The opening of internally-drained (endorheic) sedimentary basins often leads to a major drainage change, re-excavation of the basin sedimentary infill, and transient landscape. The timing of such basin openings can be dated only in exceptional cases
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6df5b0b08aeef5775088b24d789eeaf6
http://hdl.handle.net/10651/62989
http://hdl.handle.net/10651/62989
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
Publikováno v:
Gondwana Research. 42:49-62
As a proxy for long-term lithospheric strength, detailed information on lateral effective elastic thickness (Te) variations can aid in understanding the distribution pattern of surface deformation and its response to long-term forces. Here we present
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