Local H I filaments driven by a small-scale dynamo - Unraveling the velocities and tangling of dusty magnetized structures

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Fig. 23

Two-dimensional histograms of filament curvatures C in central parts of the filaments versus changes in curvature radius, characterized by the ratio R_C for channels offset from v_fil by 1, 4, and 16 km s⁻¹ (top to bottom). Displayed are the all sky data (left) and at the high latitude data (right).

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