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Fig. 4


Filled contours of simulated particle density in units cm−3 in the inner heliosphere, close to the ecliptic, ten hours after injection (11:40 UT). The locations of five observer platforms are shown along with Parker spiral connectivity using a solar wind speed of 400 km s−1. The 1 au distance is shown with a dashed circle. The arrow is placed along the radial direction at the flare location.

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