Fig. 10.
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Evolution of the erupting prominence shown in Figure 9 in 3D in heliographic coordinate system. The position of the prominence determined by joining all the reconstructed points at different instants of time, are marked on the plot. The coordinate system is centered on the Sun, with the Z-axis along the solar rotation axis, and the X-axis pointing toward the Earth (adapted from Joshi & Srivastava 2011a).
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