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Fig. 6


Oscillatory parameters of the EUV prominence, showing a) initial transverse velocity amplitude, b) period and c) initial phase, versus actual height above the solar surface; d) damping time versus period. The first oscillatory train is shown in black, and the second in red. The NE leg is indicated by triangles joined with a solid line, and the SW leg by diamonds joined with a dashed line.

This figure is made of several images, please see below:

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