Two-dimensional simulations of coronal rain dynamics - I. Model consisting of a vertical magnetic field and an unbounded atmosphere

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Fig. 1.

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Density at different times of the simulation I-5. The horizontal red dashed lines represent the position that would correspond to a free-falling object. The black asterisks show the position of the points whose kinematics is represented in Fig. 2. An animation of this figure is available online.

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