Figure 2
The He fluxes in three energy ranges (a: 0.25 - 0.5 MeV/amu, b: 0.5 - 0.75 MeV/amu, and c: 0.75 - 1.0 MeV/amu), and the spectra of suprathermal H, He, CNO, and Fe during the passage of the shock and in the following strong magnetic turbulence.