Amplified Eastward SAPS Flows Observed in the Topside Ionosphere near Magnetic Midnight

We report the exceptional observations of amplified eastward subauroral polarization streams (SAPS) made by the F15 spacecraft at ~840 km altitude near magnetic midnight during 2015–2016 in 17 events. The results show the dawn-cell-associated amplified eastward SAPS flows streaming alongside the duskward-extending dawn cell. The amplified eastward SAPS flows maximized at ~3200 m/s within their respective deep plasma density troughs, mimicking the SAPS flows and thus implying positive feedback mechanisms in action, where the electron temperature reached ~7000 K. One set of correlated magnetosphere–ionosphere conjugate observations is also presented. This illustrates the magnetotail-reconnection-related inward-directed cross-tail convection electric field (EC) reaching the near-earth plasmasheet’s tailward end, while the inward-directed SAPS E field was absent on the inner-magnetosphere plasmapause, and the emerging eastward SAPS flow in the conjugate ionosphere. These results provide observational evidence that the earthward-propagating inward-directed dawn–dusk cross-tail E field (1) mapped down to auroral latitudes with an equatorward direction, (2) propagated to subauroral latitudes, and (3) played a key role in the development of the emerging eastward SAPS flow and in the amplification of the fully-developed eastward SAPS flows near magnetic midnight, while positive feedback mechanisms supported further SAPS growth.