Timing and localization of near‐Earth tail and ionospheric signatures during a substorm onset

Abstract

On 16 February 2008, the THEMIS spacecraft (probes) bracketed the near‐Earth signatures of a substorm onset as identified in the THEMIS ground‐based observatories measuring an AE TH index up to 180 nT. The main onset was associated with the formation and tailward release of a plasmoid (a proto‐plasmoid) at X GSM = −18.3 R E and a dipolarization in the inner part of the plasma sheet at X GSM = −11.0 R E . The time history and geometry of the event in the tail are consistent with magnetic reconnection as the cause of the substorm expansion onset process. Two activations of the plasma sheet, evidenced by tailward streaming of energetic ions and southward or bipolar signatures of the magnetic field, preceded the main substorm. The first activation was associated with an intensification of a high‐latitude arc, while the second was associated with the onset of ULF pulsations at midlatitude and low‐latitude stations. We conclude that near‐Earth plasma sheet activity that may also be due to reconnection and may be related to nonsubstorm arc intensifications can precede substorm onset by several minutes. In particular, high‐latitude arcs do not appear to result in substorm initiation even though they may occur in close temporal and spatial proximity to the substorm arc.