Stabilization of the astropause by periodic fluctuations of the stellar wind

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The meaning of the name of each file is described below.

The beginning of the name of each file corresponds to Fig. 2 in the work: (b) - results with \(\bf \chi = 5\), (c) - \(\bf \chi = 10\), and (d) - \(\bf \chi = 17\). The numbers correspond to: 1 - isolines of the Mach number, 2 - isolines of the Mach number, and two plots of the Mach number versus time at two points in the inner and outer shock layer indicated on the video by a line, 3 - isolines of the density. All results are presented for \(M_\infty = 2\) (which corresponds to the heliosphere).