Regionally Extensive Hydration of the Uppermost Mantle Beneath Mars' Northern Lowlands [Code and Data]
收藏资源简介：
Code and Data for Reproducing Figures 1–3 in Regionally Extensive Hydration of the Uppermost Mantle Beneath Mars’ Northern Lowlands Overview This repository contains the codes and data required to reproduce Figures 1–3 presented in the manuscript: Shi, J., et al. A Hydrated Uppermost Mantle Beneath Mars’ Northern Lowlands. The materials are organized into separate folders corresponding to each figure. Folder Structure CodeForFigure1 Codes and data used to reproduce Figure 1. This folder contains scripts for: Plotting Martian seismic velocity models. Visualizing seismic anisotropic structures inferred from InSight observations. Generating the figure panels related to crustal and uppermost mantle structure beneath Mars. CodeForFigure2 Codes and data used to reproduce Figure 2. This folder contains scripts for: Plotting Martian topography. Plotting Bouguer gravity anomaly maps. Plotting geological maps of Mars. Generating the figure panels used for comparison between topography, gravity, and geological observations. CodeForFigure3 Codes and data used to reproduce Figure 3. This folder contains scripts for: Identifying and visualizing candidate serpentinized regions. Mapping inferred hydrated uppermost mantle reservoirs. Generating the figure panels showing the proposed distribution of serpentinization on Mars. Software Requirements The scripts were developed using Python. Required packages may include: NumPy SciPy Matplotlib ObsPy Cartopy / Basemap (depending on the specific figure) Additional dependencies are documented within individual scripts where necessary. Citation If you use these codes or data in your research, please cite: Shi, J., et al. A Hydrated Uppermost Mantle Beneath Mars’ Northern Lowlands. Please also cite this Zenodo repository. Contact Jing ShiEmail: shij@smail.nju.edu.cn
