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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 10.

Top: z-energy flux density, bottom: θ-energy flux density of the shocktube plasma. Each plot shows their respective quantities for all time at positions z = 0.3 and z = 0.99.

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