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Fig. 5

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Heliocentric dependencies of (left) the dust ejection rate, (center) the dust velocity of a0 = 1 cm-sized particles at a cometocentric distance of R = 20RN, and (right) the power index of the dust size distribution. The plots are adopted from Fig. 3 in Pozuelos et al. (2014a), while we excluded the data relevant to the two small outburst events observed in the 2010 apparition.

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