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Fig. 1


Proton temperature distribution in the dynamic heliosphere (Scherer & Ferreira 2005). Above the solar pole the features of a high-speed stream can be identified. Because of the influence of the PUISH+ the temperature inside the termination shock is a few 105 K, corresponding to thermal energies of up to a few tens of eV. The temperature in the inner heliosheath is 106 K, which was inferred by IBEX (Livadiotis et al. 2011).

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