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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 3.

(a) The termination shock and the flow lines in the heliosheath assuming a varying shock compression ratio as a function of θ angle. The ﹩{r}_{h}﹩(θ = 0°) − rs(θ = 0°) length is set to 37.6 AU and the compression ratio for θ = 0° is set to R(θ = 0°) = 15. (b) The compression ratio of the termination shock as a function of θ.

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