Impact of solar-wind turbulence on a planetary bow shock - A global 3D simulation

Open Access

Fig. 7

Transient structure along the location of the bow shock in the X-Z plane of the turbulent simulation at $t = 250 Ω_{ci}^{- 1}$ $t = 250\Omega _{{\rm{ci}}}^{ - 1}$ . (a) Ion density N_i (logarithmic scale, in units of n₀). (b) Total magnetic field intensity |B| (logarithmic scale, in units of B₀). (c) Proton bulk speed U_p (linear scale, in units of C_A, in the shock’s reference frame).

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