Velocity structure functions for a subset of M_cl ∼ 10^5.2±0.2 M_⊙ clouds in the inner halo (galactocentric distance ∼0.3 R_200c). The extreme tenth percentile of clouds were picked based on cloud radius, with the VSFs of smaller (larger) clouds shown on the left (right). Thin colored curves correspond to individual clouds, thick solid curves to median, and the vertical dashed gray line to the average cell size. Both medians and a vast majority of the individual curves follow a ∝l^1/2 scaling, suggesting that the power law slope of the VSF is k ∼ 1/2.