Martian Ion Drift and Magnetic Field Data with Supporting Code

A dataset from the Chinese Academy of Sciences includes code for Martian crustal magnetic field models and associated data files. The data likely contains traced magnetic field lines, ion pitch angle distributions, magnetic topology indices, wave properties, and curvature radius distributions. The dataset is hosted on GitHub and is associated with a scientific paper.

Use Cases

• Modeling Martian crustal magnetic fields based on the provided G110 model code.
• Analyzing ion pitch angle distributions based on the data mentioned in the description.
• Studying magnetic topology and field line curvature based on the available indices and parameters.
• Investigating wave properties in the Martian environment based on the described data.

Strengths

• Includes executable code for the Martian crustal field G110 model.
• Contains multiple data types mentioned in the paper, such as traced magnetic field lines and ion pitch angle distributions.

Limitations

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

Provenance

Source

Chinese Academy of Sciences

Collection Method

Likely derived from spacecraft measurements and numerical modeling, as described in the associated paper.

Geography

Mars