Download original image
Simulations of F-UT patterns sorted by the polarity of the average IMF [BY]GSEQ component during the prior hour. The top row shows the Russell-McPherron patterns PRM(F, UT) in normalised power input into the magnetosphere simulated using the eccentric dipole geomagnetic field model for 2002 with (a) [BY]GSEQ = +|B|, (b) [BY]GSEQ = −|B|, and (c) an equal mix of [BY]GSEQ = +|B| and [BY]GSEQ= −|B|. The middle panels show the corresponding modelled patterns of Pm(F, UT) = PRM(F, UT) · Pψ(F, UT) · PNS(UT). The observed patterns in aσ(midn) data shown in the bottom panels are for (g) [BY]GSEQ < 0, (h) [BY]GSEQ > 0 and (i) all data.
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.