The effect of turbulence strength on meandering field lines and Solar Energetic Particle event extents | Journal of Space Weather and Space Climate

Flares, coronal mass ejections and solar energetic particles and their space weather impacts

Open Access

Fig. 1

Left panel: Parallel (thick curves) and perpendicular (thin curves) particle mean free paths as function of radial distance from the Sun, for 10 MeV protons and different turbulence strengths parametrised by . Right panel: The ratio of the field line and cross-field particle diffusion coefficients.

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