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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 5.

(a) Time–distance plot of normalized vθ. The velocity is negative upon forward propagation and positive on backward propagation of the Alfvén wave. The signal is amplified at the shock location upon each reflection, with a portion of the signal being transmitted. A standing slow shock forms at the gas-dynamic shock location and can be seen as a faint, white line after t = 2 at z = 0.5. Panel (b) shows the trapped portion of the Alfvén wave at z = 0.3. The transmitted portion is shown in panel (c) for z = 0.99.

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