Fig. 6: Dynamics of the simulated MHD wave and its amplitude variations along three selected paths.
From: Resolved magnetohydrodynamic wave lensing in the solar corona

a–c Time-distance plots to show the total energy density \(\delta {{{{{{{\mathcal{H}}}}}}}}/{p}_{0}\) along the paths as shown in Fig. 5b, where \(\delta {{{{{{{\mathcal{H}}}}}}}}\) is the difference between total energy density \({{{{{{{\mathcal{H}}}}}}}}\) and the background total energy density \({{{{{{{{\mathcal{H}}}}}}}}}_{0}\). The vertical dotted lines indicate the CH boundaries in the numerical simulation. d The amplitude variation of the wavefront along the selected paths. As the upper/lower paths shown in Fig. 5b are symmetric to each other, the measured values are identical. The values of normalization factors p0, t0, and L0 for the total energy density (\({{{{{{{\mathcal{H}}}}}}}}\)), time (t) and length (x, y, z) are listed in Table 1.