https://ogma.newcastle.edu.au/vital/access/ /manager/Index ${session.getAttribute("locale")} 5 https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:3254 Wed 11 Apr 2018 17:06:56 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:3259 Wed 11 Apr 2018 16:08:23 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:17370 E. Wave polarization appeared to be associated with plasma density, with left hand in the equatorial region, right hand at higher latitudes nearer the plasmapause, and a mixture between.Wave normal angles were typically <60°, and Poynting flux measurements show that wave energy was predominantly directed along the geomagnetic field toward high latitudes in both hemispheres. These results suggest that the plasma density and its gradient play a significant role in confining the wave source region and affecting the wave properties, which will help understand wave generation and propagation mechanisms in the magnetosphere plasma environment.]]> Wed 11 Apr 2018 11:32:27 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:2003 Wed 11 Apr 2018 10:37:04 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:14033 Wed 11 Apr 2018 09:25:20 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:1121 Sat 24 Mar 2018 08:32:00 AEDT ]]>