Number of clumps as a function of angular resolution (FWHM) for the same five SINGS galaxies (NGC 2976, NGC 3938, NGC 0024, NGC 0337, and NGC 1512), with the curves once again coloured by the original seeing (FWHM). The curves are well fitted with quadratic forms (median R² = 0.995) and have a large scatter that is significantly correlated with the original angular resolution, suggesting a more complex relationship with clump properties than distance that is likely related to the angular scales associated with Scarlet scales two and three.