Fig. 6.
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Coronal holes on 7 June 2012 obtained by CHIMERA. Fast solar wind regions observed in Fig. 11 are consistent with the location of CH1. Magnetogram data from SOLIS show 10+ as the number of NOAA active regions, four of which are adjacent to the East of CH1. This is later shown to be consistent with the location of the triangulated Type III beam.
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