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Nonlinear decay of foreshock Langmuir waves in the presence of plasma inhomogeneities: Theory and Cluster observations

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    SYSNO ASEP0306673
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleNonlinear decay of foreshock Langmuir waves in the presence of plasma inhomogeneities: Theory and Cluster observations
    TitleNelineární rozpad Langmuirových vln ve slunečním větru před rázovou vlnou za přítomnosti nehomogenit plasmatu: teorie a měření družicemi Cluster
    Author(s) Souček, Jan (UFA-U) RID, ORCID
    Krasnoselskikh, V. (FR)
    Dudok de Wit, T. (FR)
    Pickett, J. (US)
    Kletzing, C. (US)
    Source TitleJournal of Geophysical Research - ISSN 0148-0227
    Roč. 110, A8 (2005), A08102/1-A08102/10
    Number of pages10 s.
    Languageeng - English
    CountryUS - United States
    Keywordsplasma waves ; kinetic waves and instabilities ; foreshock ; solar wind
    Subject RIVBL - Plasma and Gas Discharge Physics
    R&D ProjectsME 650 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA202/03/0832 GA ČR - Czech Science Foundation (CSF)
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    DOI https://doi.org/10.1029/2004JA010977
    AnnotationThe intense high frequency electrostatic waves observed in the terrestrial foreshock often have a form of a superposition of two monochromatic waves close to the plasma frequency. We suggest an interpretation of these spectra as signatures of nonlinear decay of Langmuir waves to electron-sound and ion-sound secondary waves. This decay instability is known to have different properties in inhomogeneous plasma, namely the threshold amplitude of this instability is inversely proportional to the scale of the inhomogeneity. We show that the observed dependence of the wave amplitude on the modulation scale of the wave-packets is consistent with this property and the theory of absolute decay instability in inhomogeneous plasma can be applied to explain the satellite observations. In this study we used electric field data from the WBD instrument on-board CLUSTER satellites.
    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 Publishing2008
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