Temporal evolution of axially standing kink motions in solar coronal slabs: An eigenfunction expansion approach

Open Access

Fig. 3.

Time-dependent solution obtained with eigenfunction expansion method for the combination [ρ_i/ρ_e = 5, μ = ∞, kd = π/20, Λ/d = 1]. Shown is the distribution of the lateral speed $\hat{v}$ $\hat{v}$ in the x − t plane, with the filled contours chosen to better visualize the wave dynamics at short times.

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