Fig. 9.


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Heliospheric model simulation shows the background solar wind conditions (black lines) at the Earth and the disturbed solar wind conditions upon arrival of the CME (red lines) on April 18, 2014. The green lines are solar wind observations from the ACE satellite. From top to bottom: solar wind speed (V sw), variation of solar wind speed (∆V sw), proton density (ρ), strength of magnetic field (B), polar angle of magnetic field (θ), and azimuthal angle of magnetic field (Φ).

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