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

Open Access

Fig. 7.

Velocity streamlines (white) shown for the magnetic field magnitude for the inclination angle α = 60° and for ISMF intensity 2 μG (a) Iso SW without the IMF (b) Iso SW with the IMF (c) Anis SW with the IMF.

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