Figure 9 from THE NONLINEAR EVOLUTION OF A TWIST IN A MAGNETIC SHOCKTUBE

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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 9.

The internal energy of the shocktube plasma is split into its constituents—thermal, z-kinetic, θ-kinetic, and θ-magnetic energies for z = 0.3 (brown) and z = 0.99 (purple).

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