Abstract

Abstract. The location of magnetic reconnection in the mid-tail during a substorm was studied in many researches. Here we present multi-point THEMIS observations of a reconnection event in the near-Earth magnetotail during substorm. In this event, THEMIS probes stayed in the near-Earth and mid-tail region aligning along the magnetotail. This allows reconnection evolution to be probed simultaneously from about −10 RE to −23 RE down tail. The Hall current related electron streams were observed at the same time by two probes far away from the reconnection site. Before near-Earth reconnection involved the tail lobe magnetic field, the reconnection site was restricted in earthward −23 RE. When reconnection involved into the tail lobe region, the reconnection site started to retreat gradually.

Highlights

  • Magnetic reconnection is a physical process which produces a change in magnetic field topology, and converts magnetic field energy into particle kinetic and thermal energies

  • Magnetic reconnection plays an essential role in various aspects of the formation and dynamics of the Earth’s magnetosphere (e.g. Dungey, 1961), especially in substorm physics

  • In the Near-Earth neutral line (NENL) model, a neutral line is formed and the magnetic reconnection occurs in association with a substorm

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Summary

Introduction

Magnetic reconnection is a physical process which produces a change in magnetic field topology, and converts magnetic field energy into particle kinetic and thermal energies. In the NENL model, a neutral line is formed and the magnetic reconnection occurs in association with a substorm. This causes the formations of the tailward moving plasmoids and the earthward bursty bulk flows (BBFs) which transport magnetic flux, mass and energy at a high speed. The magnetic reconnection site does not remain at the same place It retreats tailward in the late expansion or recovery phase of the substorm (Forbes et al, 1981; Angelopoulos et al, 1996), as predicted by the near-Earth neutral line (NENL) model (Hones, 1976).

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