Fig. 12
Simulated size distributions of the ISD at the main-belt asteroid Ceres for the 4 positions per orbit (cf. Fig. 4). The dotted straight line is the original reference distribution for nH = 0.3 cm-3. The black straight line is the reference distribution range for which simulations were done. This reference distribution is illustrative, and is not meant to imply that the extended MRN distribution would reflect the true grain size distribution in the LIC.
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