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

Open Access

Fig. 9.

Dependence of frequency ω_peak, 2 on Λ/d, where $| S_{ω} {\overset{˘}{v}}_{ω} (x = 0) |$ $|S_\omega {\breve{v}}_\omega(x=0)|$ attains the second peak. A fixed combination [ρ_i/ρ_e = 5, μ = 1, kd = π/20] is adopted. The hatched portion corresponds to the frequency range $[0.9, 1.1] \times R Ω_{2}^{DLM}$ $[0.9, 1.1] \times \Re\Omega^{\mathrm{DLM}}_{2}$ (see text for details).

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