Abstract

Abstract. During auroral substorms, the electric currents flowing in the ionosphere change rapidly, and a large amount of energy is dissipated in the auroral ionosphere. An important part of the auroral current system is the auroral electrojets whose profiles can be estimated from magnetic field measurements from low-earth orbit satellites. In this paper, we combine electrojet data derived from the Swarm satellite mission of the European Space Agency with the substorm database derived from the SuperMAG ground magnetometer network data. We organize the electrojet data in relation to the location and time of the onset and obtain statistics for the development of the integrated current and latitudinal location for the auroral electrojets relative to the onset. The major features of the behaviour of the westward electrojet are found to be in accordance with earlier studies of field-aligned currents and ground magnetometer observations of substorm temporal statistics. In addition, we show that, after the onset, the latitudinal location of the maximum of the westward electrojet determined from Swarm satellite data is mostly located close to the SuperMAG onset latitude in the local time sector of the onset regardless of where the onset happens. We also show that the SuperMAG onset corresponds to a strengthening of the order of 100 kA in the amplitude of the median of the westward integrated current in the Swarm data from 15 min before to 15 min after the onset.

Highlights

  • Ionospheric electric currents give rise to a variety of space weather effects that influence the performance and reliability of space-borne and ground-based technological systems.Problems in ground-based systems occur, for instance, due to geomagnetically induced currents (GIC) in technological conductor systems such as power grids (Pirjola, 2000, 2002)

  • We have shown that the auroral electrojet characteristics derived from Swarm-AEBS data products are organized in a way that can be interpreted to be consistent with earlier observations of bulge-type substorm expansion and large-scale substorm current wedge (SCW) development

  • The data consist of separate oval crossings from different sectors of substorm current systems, the resulting distribution agrees with earlier studies of the temporal development of substorms, at least in the 15 min timescale used in this study

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Summary

Introduction

Problems in ground-based systems occur, for instance, due to geomagnetically induced currents (GIC) in technological conductor systems such as power grids (Pirjola, 2000, 2002). The development of the aurora at the onset time and during substorms was first described by Akasofu (1964), who determined that, despite the variability from substorm to substorm, there are common substorm features, such as the formation and expansion of the bulge poleward, westward and eastward. Another prevalent phenomenon linked to substorms is the formation of the substorm current wedge (SCW).

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