Fig. 10.
Spatial profiles of the modelled radial velocity, number density, and HEEQ Bz-component of the magnetic field of the CME upon arrival at Venus Express orbit. The top row shows the model output for a spheromak with radius RωEO, the middle row for ⟨R⟩, and the bottom row for RωFO. Both equatorial and meridional cuts are provided to offer a perspective of what portion of the modelled CME structure crossed the spacecraft.
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