2.5D high-amplitude dipole

This simulation is part of a series of simulations of the solar wind including cosmic rays diffusion.

Simulation data

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Download VTK file: in spherical coordinates (58.8MB) or Cartesian coordinates (979MB).

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Simulation metadata

Metadata are available as a JSON file and are summarized below:

• Author: Barbara Perri
• Reference: Perri et al. (2020)
• Dimension: 2.5D (resolution: 1024×256)
• Case: High-amplitude dipole
• Magnetic field: dipole, amplitude 5 G
• Coronal temperature: 1.6 10⁶ K
• Adiabatic index: 1.05
• Rotation rate: 2.6 10^-6 s^-1
• Coronal density: 10⁸ cm^-3
• Cosmic ray rigidities: [1, 10, 100, 445, 1000, 10000, 100000] MV