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...

Full description

Bibliographic Details
Main Authors: J. S. Maia, M. A. Wieczorek, A.‐C. Plesa
Format: Article
Language:English
Published: Wiley 2023-08-01
Series:Geophysical Research Letters
Subjects:
Online Access:https://doi.org/10.1029/2023GL103847