Fig. 2.

Download original image
Solar wind and geomagnetic (aa, Kp × 10) indices for a two solar rotation interval in August–October 2003 dominated by a sequence of corotating high-speed streams with peak speeds ~600–800 km s−1. Geomagnetic activity frequently reached G1–G3 levels (bottom panel). The solar wind parameters shown are: the magnetic field intensity, polar and azimuthal angles (GSE coordinates), proton temperature with expected temperature (Richardson & Cane 1995) in red; density and solar wind speed.
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.