Open Access

Fig. 11

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Time series of relative fluxes with respect to main-belt asteroid Ceres for different grain sizes (0.73, 0.36, 0.26, 0.21, 0.15, 0.11, and 0.07 μm cf. Fig. 6). As the grain size decreases, the influence of the solar cycle becomes more dominant. Filtering at the heliopause is not taken into account.

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