Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Bart Root"'
Autor:
Weilun Qin, Bart Root
The largest volcanos in our Solar System are part of a huge volcanic complex, named Tharsis Rise, which is located on the Martian surface several kilometers higher than the average topography. Moreover, the gravitational field of Mars shows a strong
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::778208af69706ed6eb802a0098360421
https://doi.org/10.5194/egusphere-egu23-6454
https://doi.org/10.5194/egusphere-egu23-6454
The Tharsis Region has been an interest of study for many years due to its large impact on the long wavelength gravity field and topography of Mars. The leading theory on the origin of the volcanic region is a combination of both isostatic flexure of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0a2f8870c95ae12ab2baca76c4178645
https://doi.org/10.5194/egusphere-egu23-13871
https://doi.org/10.5194/egusphere-egu23-13871
Autor:
Bart Root
Flexural isostasy is commonly used to understand the relationship between the observed topography, the crustal structure, and the gravity. Compared to local isostasy, flexural models behave like low-pass filters on the crust-mantle interface. Using t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9073b5298c0920cc8ef4df93e3f5e14d
https://doi.org/10.5194/egusphere-egu23-5562
https://doi.org/10.5194/egusphere-egu23-5562
Autor:
Bart Root, Weilun Qin
Mars hosts the largest volcano in our solar system, Mons Olympus. This volcano is part of a huge volcanic complex, named Tharsis Rise, which is situated several kilometers higher than the average surface. Flexural isostasy is commonly used to underst
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::35e8bc07765c6a0bb740a519786cf8db
https://doi.org/10.5194/epsc2022-375
https://doi.org/10.5194/epsc2022-375
Rocky (exo)planets can be classified based on their mantle viscous state. The mantle viscosity influences the efficiency of convection and heat loss of the planet, altering the outgassing rate. Low viscous planets are hypothesized to have strong volc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6c172d3d67a02082a14d17c93e6dd48
https://doi.org/10.5194/epsc2022-1219
https://doi.org/10.5194/epsc2022-1219
1. Introduction With the increasing interest in the Solar System's smaller bodies, quite a few missions have been sent to comets and asteroids, and more will be send in the near future. Due to the large distances involved, communication to command mi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3f9a4f4abc2e778d10eb1c7a1ca54374
https://doi.org/10.5194/epsc2022-511
https://doi.org/10.5194/epsc2022-511
Autor:
Jesse Reusen, Pingping Huang, Rebekka Steffen, Holger Steffen, Caroline van Calcar, Bart Root, Wouter van der Wal
In geodynamic studies, most Finite-Element (FE) models in the commercial FE software Abaqus use elastic foundations at internal boundaries. This method works well for incompressible and so-called material-compressible material parameters but it is un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9ca7e29b73d25a61a8801dbe6d7ff6b3
https://doi.org/10.5194/egusphere-egu22-5146
https://doi.org/10.5194/egusphere-egu22-5146
Autor:
Bart Root
Publikováno v:
Geophysical Journal International, 221(3)
SUMMARY Current seismic tomography models show a complex environment underneath the crust, corroborated by high-precision satellite gravity observations. Both data sets are used to independently explore the density structure of the upper mantle. Howe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::65f3de5b47afd19dee1db943e4f22c48
https://doi.org/10.1093/gji/ggaa091
https://doi.org/10.1093/gji/ggaa091
