The Mantle Viscosity Structure of Venus
Abstract The long‐wavelength gravity and topography of Venus are dominated by mantle convective flows, and are hence sensitive to the planet's viscosity structure and mantle density anomalies. By modeling the dynamic gravity and topography signatures and by making use of a Bayesian inference ap...
| Váldodahkkit: | , , |
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| Materiálatiipa: | Artihkal |
| Giella: | English |
| Almmustuhtton: |
Wiley
2023-08-01
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| Ráidu: | Geophysical Research Letters |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.1029/2023GL103847 |