Meridional cuts through the Oz-V2 plane from a 3D MHD simulation showing the log of the solar wind number density (cm-3), the velocity (km s-1), the log of the temperature (K), and the magnetic field magnitude (nT) at t = 1 yr after the reverse shock crossed the TS. FS′ denotes the forward shock propagating into the heliosheath; TD1 and TD2 are tangential discontinuities; TS is the termination shock; R denotes a rarefaction wave formed after the interaction of the TS and the reverse shock.
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.