Influence of the interstellar magnetic field and 11-year cycle of solar activity on the heliopause nose location

Open Access

Fig. 2.

Schematic of the heliosphere and LISM for an ISMF not parallel to the LISM velocity vector. The TS and HP noses deviate in one direction (quasi-perpendicular to the undisturbed B_is), and the BS nose in the opposite direction (Ratkiewicz et al. 2000).

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