A three-component cosmic-ray model that includes the local interstellar cloud's motion and magnetic field reproduces the energy-dependent dipole anisotropy of cosmic rays from GeV to PeV energies, but with many fitted parameters.
For a given magnetic field B, a lower value of Rcr implies a smaller diffusion coefficient k‖ and a higher turbulence intensity
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Influence of interstellar environment near the solar system on cosmic-ray spectra and dipole anisotropy
A three-component cosmic-ray model that includes the local interstellar cloud's motion and magnetic field reproduces the energy-dependent dipole anisotropy of cosmic rays from GeV to PeV energies, but with many fitted parameters.