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Fig. 4


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 temperature (K), and the magnetic field magnitude (nT) at t = 0.7 yr when the forward shock crossed the heliospheric termination shock. FS′ denotes the forward shock propagating into the heliosheath, TD is a tangential discontinuity, TS is the termination shock, and RS is a reverse shock upstream of the TS.

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