Fig. 8.
Top row: particle intensities of energy channel 4.2 ± 0.2 MeV drawn in grey shades on top of the radial velocity profile of the solar wind. Bottom row: particle intensities of energy channel 4.6 ± 0.2 MeV drawn in grey shades on top of scaled pressure profile of the solar wind. The right and left columns correspond, respectively, to the simulations with and without perpendicular diffusion. The entire temporal evolution is available as an online movie.
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