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Breathing of heliospheric structures triggered by the solar-cycle activity

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Figure

Table 1. The parameter for the calculations, while the interstellar parameters are assumed to be valid at “infinity”
Fig. 1. The proton density variations for the static and the dynamic heliosphere (LISM flow from the right)
Fig. 2. Same as in Fig. 1 in a logarithmic scale, which enhances the effects in heliotail region.
Fig. 3. Same as in Fig. 1 for the hydrogen distribution. To enhance the effects the solar wind speed variations reach from 300 km/s to 800 km/s for a pure sinusoidal law
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