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Smoothing of MHD Shocks in Mode Conversion

  • Authors: Jamon D. Pennicott, and Paul S. Cally

2019 The Astrophysical Journal Letters 881 L21.

  • Provider: AAS Journals

Caption: Figure 2.

θ = 15°: at the a = c layer, the slow shock is smoothed slightly, before steepening again to produce another shock front. The fast shock remains sharp and propagates unaltered. The orange dot shows the location of the steepest point in the fast shock.

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