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Modeling the Plasma Flow in the Inner Heliosheath with a Spatially Varying Compression Ratio

  • Authors: G. Nicolaou, and G. Livadiotis

2017 The Astrophysical Journal 838 7.

  • Provider: AAS Journals

Caption: Figure 1.

Representation of ﹩{\alpha }_{1},{\alpha }_{s}﹩ and ﹩\varphi ={\alpha }_{s}-{\alpha }_{1}﹩ angles. The red solid line represents the termination shock surface, while the dashed red line represents the shock normal. The plasma downstream flow vector is represented with the blue arrow.

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