THE NONLINEAR EVOLUTION OF A TWIST IN A MAGNETIC SHOCKTUBE
Authors: Thomas Williams, Youra Taroyan, and Viktor Fedun
2016 The Astrophysical Journal81792.
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.