Number of the records: 1  

Oblique lower band chorus waves: Time shifts between discrete elements observed by the Cluster spacecraft

  1. 1.
    SYSNO ASEP0335031
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleOblique lower band chorus waves: Time shifts between discrete elements observed by the Cluster spacecraft
    TitleŠikmo se šířící chorové vlny spodního pásu: časové posuvy mezi diskrétními elemnty pozorovanými družicemi Cluster
    Author(s) Chum, Jaroslav (UFA-U) RID, ORCID
    Santolík, Ondřej (UFA-U) RID, ORCID
    Gurnett, D. A. (US)
    Pickett, J. S. (US)
    Source TitleJournal of Geophysical Research - ISSN 0148-0227
    Roč. 114, - (2009), A00F02/1-A00F02/13
    Number of pages13 s.
    Languageeng - English
    CountryUS - United States
    Keywordsplasma waves ; wave particle interaction ; inner magnetosphere ; radiation belt
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsGA205/09/1253 GA ČR - Czech Science Foundation (CSF)
    IAA301120601 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000272946500001
    DOI10.1029/2009JA014366
    AnnotationWe report observations of remarkable frequency differences and time shifts between the corresponding elements of lower band chorus recorded by the four Cluster spacecraft at low magnetic latitudes. Surprisingly, the spacecraft located closer to the equator systematically received the corresponding chorus elements later than the spacecraft located at higher magnetic latitudes. The time shifts and frequency differences depended almost linearly on the perpendicular distance between the various spacecraft. Analysis of data shows that chorus emissions were generated with highly oblique angles of propagation. We show that the sources moving across the magnetic field lines are reasonably consistent with these observations. We propose that the transverse motion of the chorus sources is a consequence of a feedback between the oblique waves and counter streaming electrons during nonlinear cyclotron interactions, and we provide an estimate of the transverse velocity of the source.
    WorkplaceInstitute of Atmospheric Physics
    ContactKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Year of Publishing2010
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.