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Fig. 12.


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The logarithm of the proton peak fluxes (in pfu) at several integral energies (E > 10 [A]; >30 [B]; >60 [C] and >100 MeV [D]) as a function of the plane-of-sky speed for the CMEs associated with SEP events in the SEP part of the database. The lines at each panel represent the linear fit to the data. Each panel, further, presents the correlation coefficient (cc), the respective standard error (SE) and the linear fit to the data.

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