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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 4.

θ = 60°: heavy smoothing of the slow shock through a = c. The fast shock remains sharp and propagates freely again. The transmitted slow wave is subsonic and much too weak to re-shock before the fast shock reaches the top of the computational box.

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