• → 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

    On nonstationarity and rippling of the quasiperpendicular zone of the Earth bow shock: Cluster observations

    Publication date: 23 Sep 2008

    Authors: Lobzin, V.V. et al.

    Journal: Ann. Geoph.
    Volume: 26
    Issue: 9
    Page: 2899-2910
    Year: 2008

    Copyright: EGU

    A new method for remote sensing of the quasiperpendicular part of the bow shock surface is presented. The method is based on analysis of high frequency electric field fluctuations corresponding to Langmuir, upshifted, and downshifted oscillations in the electron foreshock. Langmuir waves usually have maximum intensity at the upstream boundary of this region. All these waves are generated by energetic electrons accelerated by quasiperpendicular zone of the shock front. Nonstationary behavior of the shock, in particular due to rippling, should result in modulation of energetic electron fluxes, thereby giving rise to variations of Langmuir waves intensity. For upshifted and downshifted oscillations, the variations of both intensity and central frequency can be observed. For the present study, WHISPER measurements of electric field spectra obtained aboard Cluster spacecraft are used to choose 48 crossings of the electron foreshock boundary with dominating Langmuir waves and to perform for the first time a statistical analysis of nonstationary behavior of quasiperpendicular zone of the Earth's bow shock. Analysis of hidden periodicities in plasma wave energy reveals shock front nonstationarity in the frequency range 0.33 fBi < f < fBi, where fBi is the proton gyrofrequency upstream of the shock, and shows that the probability to observe such a nonstationarity increases with Mach number. The profiles observed aboard different spacecraft and the dominating frequencies of the periodicities are usually different. Hence nonstationarity and/or rippling seem to be rather irregular both in space and time rather than resembling a quasiregular wave propagating on the shock surface.

    Link to Publication

    Last Update: 06 Oct 2008

    • Shortcut URL
    • http://sci.esa.int/jump.cfm?oid=43521

    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