• → European Space Agency

    • About Science & Technology

    • For Public

    • For Educators

    • ESA

    • Science & Technology

    • Cluster

    • Missions
    • Show All Missions
    • Mission Home
    • Summary
    • Fact Sheet
    • Objectives
    • Mission Team
    • Orbit View
    • Background Science
    • Earth's Magnetic Field
    • Plasma Regions
    • Solar Wind
    • Energetic Particles
    • Space Weather
    • Science Results
    • Highlights
    • Refereed Publications
    • Spacecraft…

      • Spacecraft
      • 3D Model
      • Instruments
      • Engineering
    • Mission Operations…

      • Mission Operations
      • Launch Vehicle
      • Launch Campaign
      • Orbit/Navigation
      • Mission Timeline
      • Status Reports
    • Science Operations
    • Science Operations
    • Guest Investigator Operations
    • JSOC
    • CSDS
    • Cluster Active Archive
    • Resources
    • News Archive
    • Multimedia Gallery
    • Publication Archive
    • Calendar of Events
    • Services
    • Contact Us
    • Subscribe
    • Terms and Conditions
    • Bookmark and Share

    Average properties of the magnetic reconnection ion diffusion region in the Earth's magnetotail: The 2001–2005 Cluster observations and comparison with simulations

    Publication date: 14 Aug 2010

    Authors: Eastwood, J.P. et al.

    Journal: Journal of Geophysical Research
    Volume: 115
    Page: A08215
    Year: 2010

    Copyright: American Geophysical Union

    Magnetic reconnection plays a key role in the circulation of plasma through the Earth's magnetosphere. As such, the Earth's magnetotail is an excellent natural laboratory for the study of reconnection and in particular the diffusion region. To address important questions concerning observational occurrence rates and average properties, the Cluster data set from 2001-2005 has been systematically examined for encounters with reconnection X lines and ion diffusion regions in the Earth's magnetotail. This survey of 175 magnetotail passes resulted in a sample of 33 correlated field and flow reversals. Eighteen events exhibited electric and magnetic field perturbations qualitatively consistent with the predictions of antiparallel Hall reconnection and could be identified as diffusion region encounters. The magnitudes of both the Hall magnetic and electric field were found to vary from event to event. When normalized against the inflow magnetic field and the current sheet number density the average peak Hall magnetic field was found to be 0.39 ± 0.16, the average peak Hall electric field was found to be 0.33 ± 0.18, and the average out of plane (reconnection) electric field was found to be <0.04. Good quantitative agreement was found between these results and a large, appropriately renormalized particle-in-cell simulation of reconnection. In future missions, the magnitude of the total DC electric field may be a useful tool for automatically identifying ion diffusion region encounters.

    Link to Publication

    Last Update: 07 Sep 2010

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=47671

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Livestream
    • Subscribe
    • App Store
    • ESA Science Twitter

    Follow ESA science

    • Copyright 2000 - 2013 © European Space Agency. All rights reserved.

    • Terms and Conditions