The effects of expansion and turbulence on the interplanetary evolution of a magnetic cloud

Open Access

Fig. 7.

Time evolution of the maximum of u_x and minimum of u_y (both computed across a 1D cut passing through the axis, as in Fig. 4) for runs A2-A6. The trends of $u_{x}^{\max}$ $u_x^\mathrm {max}$ and $u_{y}^{\min}$ $u_y^\mathrm {min}$ are drawn with blue and orange lines respectively, with lighter shades corresponding to higher values of ɛ₀ as in Fig. 6.

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