Fig. 4
Scatter plots of the period P (upper panels) and damping time τ (lower panels) of the prominences in the oscillation step as functions of l, h, D, w, and v0. The values of P and τ in the cases | v0 | = 70 and 80 km s-1 that cause mass drainage at the footpoint of the coronal loop are marked with triangles in the right panels.
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