Abstract
Abstract. Substorm auroras observed on 17 January 1994 were localized within the field of view of an all-sky imager installed at Dawson City (DWS, 65.7° ILAT). In association with the enhancement of the anti-sunward convection in the polar cap and the ion flux enhancement in 1–6 keV at geosynchronous altitudes, a wave-like structure propagating equatorward to the onset latitudes with a high wave number in azimuth (m ~ 76, T ~ 120 s) was observed 30 min prior to the activation in the equatorward latitudes. The activation of the auroras in the equatorward latitudes and the subsequent poleward expansion lasted for approximately 6 min until a diffuse aurora formed. The auroras in the last 6 min were isolated and localized within the field of view of DWS, from 400 km west to 400 km east, and accompanied the magnetic pulse at the optical station. The magnetic pulse is interpreted by the propagating ionospheric current loop with a size comparable to the isolated auroras (~ 1000 km). We conclude that the wave-like structures in the pre-onset interval relate to the intrusion of the plasma-sheet plasmas from the tail by the convection. The plasmas from the tail eventually developed the ionospheric loop currents at the onset latitudes, in association with the triggering of the bead-like rippling of auroras and subsequent breaking out from the onset latitudes.
Highlights
Pi2 pulsations are periodic (50–170 s) oscillations of short duration (∼ 15 min) observed in geomagnetic fields, particle flux, and in auroral luminosity related to the substorm expansion (Saka et al, 1999; Solovyev et al, 2000; Shiokawa et al, 2002)
The periodic intensification of the electrojet, an ionospheric part of the substorm current wedge (SCW), is considered a source of the Pi2 signals associated with the auroral intensifications in the expansion phase (Nishimura et al, 2012)
That the SCW is composed of a number of localized current elements
Summary
Pi2 pulsations are periodic (50–170 s) oscillations of short duration (∼ 15 min) observed in geomagnetic fields, particle flux, and in auroral luminosity related to the substorm expansion (Saka et al, 1999; Solovyev et al, 2000; Shiokawa et al, 2002). The periodic intensification of the electrojet, an ionospheric part of the SCW, is considered a source of the Pi2 signals associated with the auroral intensifications in the expansion phase (Nishimura et al, 2012) It is argued, that the SCW is composed of a number of localized current elements. O. Saka et al.: Pre-onset auroral signatures and subsequent development of substorm auroras as a cavity/wave-guide mode (Allan et al, 1996). The cavity/wave-guide mode is used to explain Pi2s, both within the plasmasphere (Takahashi et al, 1992 and references in Keiling and Takahashi, 2011) and outside the plasmapause (Kim et al, 2005; Teramoto et al, 2008) These two Pi2 models, an ionospheric current model and a cavity/wave-guide model, have been discussed individually. This case study shows that fresh plasmas from the tail eventually developed the vortical currents in the ionosphere
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