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

Open Access

Fig. 10.

Magnetic fieldlines (black) shown for the magnetic field magnitude for the inclination angle α = 60° and for ISMF intensity 4 μG (a) Iso SW without the IMF (compare to Figs. 8a and 9b) (b) Iso SW with the IMF (compare to Figs. 8c and 9c) (c) Anis SW with the IMF (compare to Figs. 8d and 9e).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.