Kelvin-Helmholtz Stability Analysis Based on Dipole Tilt and Solar Wind Properties

Kelvin-Helmholtz instabilities facilitate mass and momentum transport across Earth's magnetopause boundary. This dataset likely contains results from a simplified model analyzing how stability depends on Earth's dipole tilt and interplanetary magnetic field orientation. The 1.3 GB dataset was authored by Xuanye Ma and last updated on April 9, 2026.

Use Cases

• Modeling magnetopause stability based on seasonal dipole tilt variations mentioned in the description
• Analyzing Kelvin-Helmholtz instability occurrence biases based on solar wind and IMF orientation
• Investigating mass and momentum transport across planetary boundaries based on the described parabolic magnetopause geometry

Strengths

• Dataset size is 1.3 GB, suggesting substantial model output.
• License is CC-BY-4.0, allowing for open sharing and reuse.
• Last updated date is April 9, 2026, indicating recent maintenance.

Limitations

• Row count is unknown, which may limit suitability assessment.
• Column-level documentation is absent; field semantics must be inferred after download.
• Sample data is unavailable, preventing preview of data structure.

Provenance

Source

figshare

Collection Method

Likely contains results from a simplified model of solar wind, IMF, and Earth's dipolar magnetic field.

Freshness

Last updated 2026-04-09 04:15:46