Simulation Data for Porous Convection with Internal Heating, an Enceladus Model

Source codes and output data from simulations of porous convection with internal heating, an idealized model for hydrothermal activity on Saturn's moon Enceladus. The archive was created by Thomas Le Reun of the University of Cambridge and includes Jupyter notebooks for plotting the output data. The specific number of simulations, rows, and file size are not detailed in the provided metadata.

Use Cases

• Validate and extend porous convection models based on the provided simulation output data.
• Study the dynamics of internally heated fluid flow in porous media, as described for Enceladus.
• Reproduce and visualize simulation results using the included Jupyter notebooks for plotting.
• Benchmark new numerical methods against the provided simulation source codes.

Strengths

• Includes both the simulation source codes and the resulting output data, enabling full reproducibility.
• Provides Jupyter notebooks specifically for plotting and visualizing the simulation results.
• Authored by a researcher from the University of Cambridge, suggesting an academic research origin.

Limitations

• Column-level documentation is absent; field semantics must be inferred after download.
• Row count and total data size are unknown, which may limit suitability assessment.
• Last update date is unknown; freshness unverified.

Provenance

Source

Thomas Le Reun, University of Cambridge

Collection Method

Computational simulation output