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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 3.

(a) Time–distance plot for normalized density, ρ. The density upstream of the gas-dynamic shock increases and propagating shocks are seen here, as with Figure 4. (b) The amplitude increase for the propagating secondary waves/shocks can be seen as a consequence of the Alfvén instability at z = 0.3. Panel (c) shows the downstream density at z = 0.99.

(Animations (a and b) of this figure are available.)

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

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