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THE NONLINEAR EVOLUTION OF A TWIST IN A MAGNETIC SHOCKTUBE

  • Authors: Thomas Williams, Youra Taroyan, and Viktor Fedun

2016 The Astrophysical Journal 817 92.

  • Provider: AAS Journals

Caption: Figure 4.

(a) Time–distance plot of the normalized longitudinal velocity, vz. It can be seen that the gas-dynamic shock remains stationary until propagating fast shocks form. Here, the shock is impelled along the z-direction by each shock that “hits” the gas-dynamic shock. (b) The flow speed upstream of the shock (z = 0.3) decreases as it is converted into twisting motions. Panel (c) shows the flow speed at z = 0.99.

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

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