Fig. 2.
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Number of weekly observed MHs as a function of the cruising time of BepiColombo. Panel A: solar F10.7 flux for each identified MH. Panel B: radial distance of BepiColombo to the Sun for each MH. Panel C: histogram of the number of events observed per week, with the overplotted red line showing a smoothing of the numbers over 4 weeks.
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