Download original image
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).
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.