Transitions between states of magnetotail–ionosphere coupling and the role of solar wind dynamic pressure: the 25 July 2004 interplanetary CME case

Abstract

Abstract. In a case study, we investigate transitions between fundamental magnetosphere-ionosphere (M-I) coupling modes during storm-time conditions (SYM-H between −100 and −160 nT) driven by an interplanetary coronal mass ejection (ICME). We combine observations from the near tail, at geostationary altitude (GOES-10), and electrojet activities across the auroral oval at postnoon-to-dusk and midnight. After an interval of strong westward electrojet (WEJ) activity, a 3 h long state of attenuated/quenched WEJ activity was initiated by abrupt drops in the solar wind density and dynamic pressure. The attenuated substorm activity consisted of brief phases of magnetic field perturbation and electron flux decrease at GOES-10 near midnight and moderately strong conjugate events of WEJ enhancements at the southern boundary of the oval, as well as a series of very strong eastward electrojet (EEJ) events at dusk, during a phase of enhanced ring current evolution, i.e., enhanced SYM-H deflection within −120 to −150 nT. Each of these M-I coupling events was preceded by poleward boundary intensifications and auroral streamers at higher oval latitudes. We identify this mode of attenuated substorm activity as being due to a magnetotail state characterized by bursty reconnection and bursty bulk flows/dipolarization fronts (multiple current wedgelets) with associated injection dynamo in the near tail, in their braking phase. The latter process is associated with activations of the Bostrøm type II (meridional) current system. A transition to the next state of M-I coupling, when a full substorm expansion took place, was triggered by an abrupt increase of the ICME dynamic pressure from 1 to 5 nPa. The brief field deflection events at GOES-10 were then replaced by a 20 min long interval of extreme field stretching (B z approaching 5 nT and B x ≈ 100 nT) followed by a major dipolarization ( B z ≈ 100 nT). In the ionosphere the latter stage appeared as a "full-size" stepwise poleward expansion of the WEJ. It thus appears that the ICME passage led to fundamentally different M-I coupling states corresponding to different levels of dynamic pressure (P dyn ) under otherwise very similar ICME conditions. Full WEJ activity, covering a wide latitude range across the auroral oval in the midnight sector, was attenuated by the abrupt dynamic pressure decrease and resumed after the subsequent abrupt increase.

New DMSP database of precipitating auroral electrons and ions

“…Researchers have developed and used auroral boundaries to organize energy inputs and the ionospheric response [Gussenhoven et al, 1983;Sotirelis and Newell, 2000;Redmon et al, 2010Redmon et al, , 2012aRedmon et al, , 2012bRedmon et al, , 2014Ieda et al, 2014] and to organize field-aligned currents (FACs) [Ohtani et al, 2010;Wing et al, 2010;Kilcommons et al, 2017]. Several studies have used multiple DMSP space environment instruments to further characterize the electrodynamics of the auroral zones [e.g., Anderson, 2012;Knipp et al, 2013;Redmon et al, 2014;Deng et al, 2015;Sandholt et al, 2015]. In this section, we will review a subset of these efforts, highlight findings supported by the new data set, and provide suggestions how the new SSJ data set may spur future revelations.…”