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Figure 2.
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Radial distances at which Proxima Centauri’s termination shock is located in the ecliptic plane as function of azimuth, as yielded by the 3D MHD modelling presented by Engelbrecht et al. (2024), and employed in this study. Note that the astrospheric nose is located at 0°, and the tail at 180° azimuth.
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