Accelerating the Discovery of Steady‐States of Planetary Interior Dynamics With Machine Learning
Abstract Simulating mantle convection often requires reaching a computationally expensive steady‐state, crucial for deriving scaling laws for thermal and dynamical flow properties and benchmarking numerical solutions. The strong temperature dependence of the rheology of mantle rocks causes viscosity...
Saved in:
| Main Authors: | Siddhant Agarwal, Nicola Tosi, Christian Hüttig, David S. Greenberg, Ali Can Bekar |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Wiley
2025-03-01
|
| Series: | Journal of Geophysical Research: Machine Learning and Computation |
| Subjects: | |
| Online Access: | https://doi.org/10.1029/2024JH000438 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Stable Stratification of the Helium Rain Layer Yields Vastly Different Interiors and Magnetic Fields for Jupiter and Saturn
by: S. Markham, et al.
Published: (2024-01-01) -
Improving Porosity Calculation Methods and Proposing a New Model Universally Applicable to Large- and Medium-sized Planetary Objects
by: Imre Kisvárdai, et al.
Published: (2025-01-01) -
Interior and Gravity Field Models for Uranus Suggest a Mixed-composition Interior: Implications for the Uranus Orbiter and Probe
by: Zifan Lin, et al.
Published: (2025-01-01) -
Jupiter’s Interior with an Inverted Helium Gradient
by: N. Nettelmann, et al.
Published: (2025-01-01) -
The role of thermal density currents in the generation of planetary magnetic fields
by: Mauro Bologna, et al.
Published: (2025-02-01)