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Figure 11


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Solar wind conditions and geomagnetic activity on 1 August 2011, from the OMNI database. (a) Interplanetary magnetic field (IMF), with the total field magnitude in black, and the By and Bz components in blue and red, respectively. (b) IMF clock angle. (c) Solar wind speed. (d) Solar wind density. (e) Solar wind temperature. (f) SYM-H index (red line) and AE index (black line). The shaded area corresponds to a period during which the solar wind driving conditions were relatively similar to those used as a driver of the Vlasiator run.

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