Magnetospheric Fast Magnetosonic Wave Ray Paths with Plasmaspheric Plume Effects

Simulated ray paths for Fast Magnetosonic waves in Earth's magnetosphere under conditions with and without a plasmaspheric plume. Data is stored in MATLAB .mat files, organized to reproduce specific figures from the associated research. The dataset was authored by Jiang Yu and shared via the paperswithcode platform.

Use Cases

• Compare wave propagation paths based on initial azimuthal angles from 0° to 350° with 10° spacing.
• Analyze the impact of a plasmaspheric plume on wave migration based on the 'plume' and 'noplume' data fields.
• Study frequency-dependent ray paths at four different frequencies as stored in the 'figure2_data' struct.
• Investigate the effect of initial launching local time (MLT) on wave migration from data in 'figure3_data' and 'figure4_data'.

Strengths

• Data is structured to directly reproduce four specific research figures, providing clear context for use.
• Includes comparative scenarios for magnetospheric conditions with and without a plasmaspheric plume.
• Systematic parameter variation is present, such as azimuthal angles sampled at 10° intervals from 0° to 350°.

Limitations

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

Provenance

Source

paperswithcode

Collection Method

Likely contains results from numerical simulations of magnetospheric wave propagation.