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. 7

The Gaussian σ_φ,⁡max fitted to the 10 MeV SEP maximum intensity at 1 AU during the first 10 h of the event, as a function of mean free path (green circles). The blue curve depicts the trend expected for particles propagating along meandering field lines.

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