Simulation Results on Electrostatic Charging of Lunar Cavities Governed by the Flow-to-Thermal Speed Ratio: 3D PIC Simulations and a Free-Fall Model
Authors/Creators
- 1. Graduate School of System Informatics, Kobe University
- 2. Department of Physics, University of Oslo
Description
Here we present the numerical simulation data from Nakazono and Miyake (2025), titled "Electrostatic Charging of Lunar Cavities Governed by the Flow-to-Thermal Speed Ratio: 3D PIC Simulations and a Free-Fall Model."
Table of contents (English)
All ZIP archives must be unpacked before running the notebook.
1. data.zip
Simulation outputs. One directory per run, each containing:
- plasma.inp – run parameters
- *.h5 – HDF5 snapshot used for the plots
2. plot.ipynb
This Jupyter Notebook contains scripts for visualizing the data corresponding to the figures in the paper. The scripts are designed to facilitate the reproduction of plots.
3. requirements.txt
Python packages needed for the notebook. Install with
pip install -r requirements.txt
4. scmodel.zip
Python code for the semi-analytical model called from plot.ipynb.
5. csv.zip
CSV tables of solar-wind speed and temperature extracted from
Echim et al. (2011). Used by the notebook to draw reference lines.
Notes (English)
Files
plot.ipynb
Files
(196.0 MB)
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Additional details
Funding
Dates
- Created
-
2025-06-20
Software
- Repository URL
- https://github.com/Nkzono99/emout
- Programming language
- Python
- Development Status
- Active