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...

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書目詳細資料
Main Authors: J. S. Maia, M. A. Wieczorek, A.‐C. Plesa
格式: Article
語言:English
出版: Wiley 2023-08-01
叢編:Geophysical Research Letters
主題:
在線閱讀:https://doi.org/10.1029/2023GL103847