Fig. 11.
Meridional and equatorial cuts for the modelled radial velocity, number density, and HEEQ Bz-component of the magnetic field of the CME upon arrival at STEREO-A orbit. The order of placement is based on the increasing radius of the spheromak CME from the top to bottom row (RωEO, ⟨R⟩, and RωFO). The format is the same as in Fig. 10.
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