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Fig. 3.

image

Intensity and anisotropy time profiles for different energy channels of protons injected with an initial energy of 4 MeV. All the effects of the FTE are included. The first row shows the profiles for observer A located in the slow (panel A) and fast (panel B) solar wind. The last row shows the profiles for corotating observers C (panel C) and D (panel D).

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