Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Iris, van Zelst"'
Autor:
Sara Aniko Wirp, Alice-Agnes Gabriel, Maximilian Schmeller, Elizabeth H. Madden, Iris van Zelst, Lukas Krenz, Ylona van Dinther, Leonhard Rannabauer
Publikováno v:
Frontiers in Earth Science, Vol 9 (2021)
Physics-based dynamic rupture models capture the variability of earthquake slip in space and time and can account for the structural complexity inherent to subduction zones. Here we link tsunami generation, propagation, and coastal inundation with 3D
Externí odkaz:
https://doaj.org/article/b9132b553bc64523adb7f49126042f7d
Autor:
Lognonné, Philippe, Zongbo, Xu, Elvira, Astafyeva, Marouchka, Froment, Raphael, Garcia, Taichi, Kawamura, Attila, Komjathy, Siddharth, Krishnamoorthy, Ralph, Lorenz, David, Mimoun, Naomie, Murdoch, Keisuke, Onodera, Mark, Panning, Lucie, Rolland, Iris, van Zelst
Publikováno v:
XXVIII General Assembly of the International Union of Geodesy and Geophysics (IUGG)
On the Earth, with more than a century of seismology and on Mars, with the recent InSight seismic data, seismic signals generated through the coupling of the atmosphere with interior have been detected after atmospheric explosions, either due to coup
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7714bdaf208cb0e47fef91a26d7bd5b
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5021449
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5021449
Autor:
Alessandro Regorda, Cedric Thieulot, Iris van Zelst, Zoltán Erdös, Julia Maia, Susanne Buiter
Venus is a terrestrial planet with dimensions similar to the Earth and, although it is generally assumed that it does not host plate-tectonics, there are indications that Venus might have experienced, or still does experience, some form of tectonics.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c9c2c535b2c38739743fc21bc9486fa5
https://doi.org/10.5194/egusphere-egu23-15108
https://doi.org/10.5194/egusphere-egu23-15108
The dense atmosphere of Venus and the planet’s young surface, dominated by volcanic features, bear witness to its past and potentially ongoing volcanic activity. While unique among the terrestrial planets of our Solar System, Venus is likely simila
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d787065430dad451514fcbc0909ba7bb
https://doi.org/10.5194/egusphere-egu23-8996
https://doi.org/10.5194/egusphere-egu23-8996
Autor:
Iris van Zelst, Julia Maia, Moritz Spühler, Ana-Catalina Plesa, Raphaël F. Garcia, Richard Ghail, Anna J. P. Gülcher, Anna Horleston, Taichi Kawamura, Sara Klaasen, Philippe Lognonné, Csilla Orgel, Mark Panning, Leah Sabbeth, Krystyna Smolinksi
With the selection of multiple missions to Venus by NASA and ESA planned to launch in the coming decade, we will greatly improve our understanding of Venus as a planet. However, the selected missions cannot tell us anything about the seismicity on Ve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::7e35e1e7b136b52d134ae952933bcf3b
https://doi.org/10.5194/egusphere-egu23-9086
https://doi.org/10.5194/egusphere-egu23-9086
Autor:
Silvia Brizzi, Thorsten Becker, Claudio Faccenna, Whitney Behr, Iris van Zelst, Luca Dal Zilio, Ylona van Dinther
It is widely recognized that sediments play a key role for subduction. For example, sediments subducted along the shallow seismogenic plate interface are thought to influence seismic coupling and the occurrence of megathrust earthquakes, as well as t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfa590b91caedd26f45b5bed711e2b9b
https://doi.org/10.5194/egusphere-egu23-5221
https://doi.org/10.5194/egusphere-egu23-5221
There is a growing consensus that Venus is seismically active, although its level of seismicity could be very different from that of Earth due to the lack of plate tectonics. Here, we estimate upper and lower bounds on the expected annual seismicity
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::051f3bcccf223c9d1e85b8e95df4607e
https://doi.org/10.31223/x5dq0c
https://doi.org/10.31223/x5dq0c
Autor:
Alessandro Regorda, Cedric Thieulot, Iris van Zelst, Zoltán Erdős, Julia Maia, Susanne Buiter
Publikováno v:
Journal of Geophysical Research: Planets
Venus is a terrestrial planet with dimensions similar to the Earth, but a vastly different geodynamic evolution, with recent studies debating the occurrence and extent of tectonic-like processes happening on the planet. The precious direct data that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9b7d3534fb4c6b744f51e830aee0e32
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5019071_1/component/file_5019396/5019071.pdf
https://gfzpublic.gfz-potsdam.de/pubman/item/item_5019071_1/component/file_5019396/5019071.pdf
Autor:
Iris Van Zelst
Byrne & Krishnamoorthy (2022) estimated the frequency of volcanic eruptions on Venus by scaling the eruption frequency obtained from a database containing Earth data. In reproducing their study, I found that the estimated number of new and ongoing vo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::975ddba2b98974487681b83b7b99fc88
https://elib.dlr.de/191464/
https://elib.dlr.de/191464/