• → 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

    Arrival of interplanetary shock

    Date: 11 Mar 2010
    Satellite: Cluster
    Copyright: Credit: Image courtesy of Q.-G. Zong, Peking University, China & University of Massachusetts Lowell, USA)

    This figure dramatically illustrates the effect on the Earth's magnetosphere of the arrival of an interplanetary shock. A huge increase in the number of energetic electrons and in the intensity of the electric field is clearly seen to coincide with the arrival of the shock front.

    From top to bottom: (panel a) energetic electron spectrum recorded by one of the Cluster spacecraft (C1) on 7 November 2004 from 1800 to 1900 UT; electron spatial distributions measured by the other three Cluster spacecraft C2 (panel b), C3 (panel c) and C4 (panel d) with the electric field overplotted as a black line, and (panel e) Bz magnetic field component measured on all 4 spacecraft. The dashed red vertical line marks the time of arrival of the shock-induced field disturbances.


    Last Update: 11 Mar 2010

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=46691
    • Latest selection
    • Waves in the magnetic reconnection region
    • The magnetic reconnection region in Earth's magnetosphere
    • Energy transferred by bursty bulk flows
    • Image Hi-Res Versions
    • Hi-Res [tiff]
      570.97 kb.
    • Hi-Res [jpg]
      497.49 kb.
    • See also
    • Shocking recipe for 'killer electrons'

    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