3D at minimum of activity (October 1995)

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 (228MB) or Cartesian coordinates (390MB).

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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: 3D (resolution: 128×64×128)
• Case: Minimum of activity
• Input: modes up to lmax = 15 of map Br_wilcox1995.82.c (1995-10, Carrington rotation 1902)
• 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