https://ogma.newcastle.edu.au/vital/access/ /manager/Index ${session.getAttribute("locale")} 5 https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:1995 Wed 11 Apr 2018 15:11:38 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:2808 Wed 11 Apr 2018 14:52:36 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:1996 1.3 km s⁻¹ (>77 mVm⁻¹) occurred during a ~ 5-min velocity spike, peaking at 10:40 UT during the expansion phase. The drifts decayed rapidly to ~ 300 ms⁻¹ (18 mVm⁻¹) during the 6-min recovery phase interval, 11:04 to 11:10 UT. Overall, the AWFC had a lifetime of 74 min, and was located near -65° Λ in the evening sector west of the Harang discontinuity. The large westward drifts were confined to a geographic zonal channel of longitudinal ex-tent >20° (>1.3 h magnetic local time), and latitudinal width ~2° Λ. Using a half-width of ~ 100 km in latitude, the peak electric potential was >7.7 kV. However, a transient velocity of >3.1 km s⁻¹ with potential >18.4 kV was observed further poleward at the end of the recovery phase. Auroral oval boundaries determined using DMSP measurements suggest the main flow channel overlapped the equatorward boundary of the diffuse auroral oval. During the ~ 2-h interval following the flow channel, an ~ 3° Λ wide band of scatter was observed drifting slowly toward the west, with speeds gradually decaying to ~ 50 ms⁻¹ (3 mVm ⁻¹). The scatter was observed extending past the Harang discontinuity, and had Doppler signatures characteristic of the main ionospheric trough, implicating the flow channel in the further depletion of F-region plasma. The character of this scatter was in contrast with the character of the scatter drifting toward the east at higher latitude.]]> Wed 11 Apr 2018 10:35:42 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:480 Thu 25 Jul 2013 09:09:53 AEST ]]> https://ogma.newcastle.edu.au/vital/access/ /manager/Repository/uon:1089 Sat 24 Mar 2018 08:32:11 AEDT ]]>