https://ogma.newcastle.edu.au/vital/access/ /manager/Index en-au 5 https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:4432 65 degrees during northward IMF; there is marked contrast between currents for northward and southward IMF but the evolution of the patterns is continuous with IMF rotation. The directions of flows inferred from the most poleward currents are more consistent with theoretical expectations of transport away from magnetopause reconnection than previous results. We attribute the differences to the restriction in this analysis to intervals having relatively stable distributions of current so that the data set corresponds more nearly to pure states of the system.]]> Wed 11 Apr 2018 15:05:45 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:1992 Wed 11 Apr 2018 14:29:33 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:418 Wed 11 Apr 2018 12:41:32 AEST ]]>