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Fig. 4.

image

Left panels: time evolution of the volume-averaged perturbed (a) kinetic energy in the X − Y plane , (b) magnetic energy in the X − Y plane , (c) axial kinetic energy , and (d) axial magnetic energy for the UNI-A and HEL2-A cases. Right panels: time evolution of the corresponding energies for their higher sonic Mach number (Ms = 5.00) counterparts.

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