Počet záznamů: 1  

Quasiperiodic emissions observed by the Cluster spacecraft and their association with ULF magnetic pulsations

  1. 1.
    SYSNO ASEP0423087
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevQuasiperiodic emissions observed by the Cluster spacecraft and their association with ULF magnetic pulsations
    Tvůrce(i) Němec, F. (CZ)
    Santolík, Ondřej (UFA-U) RID, ORCID
    Pickett, J. S. (US)
    Parrot, M. (FR)
    Cornilleau-Wehrlin, N. (FR)
    Celkový počet autorů5
    Zdroj.dok.Journal of Geophysical Research-Space Physics. - : Wiley - ISSN 2169-9380
    Roč. 118, č. 7 (2013), s. 4210-4220
    Poč.str.11 s.
    Forma vydáníTištěná - P
    Jazyk dok.eng - angličtina
    Země vyd.US - Spojené státy americké
    Klíč. slovaiInterplanetary shocks ; instruments and techniques
    Vědní obor RIVBL - Fyzika plazmatu a výboje v plynech
    CEPGAP205/10/2279 GA ČR - Grantová agentura ČR
    Institucionální podporaUFA-U - RVO:68378289
    UT WOS000325073600024
    DOI10.1002/jgra.50406
    AnotaceQuasiperiodic (QP) emissions are electromagnetic waves at frequencies of about 0.5–4 kHz characterized by a periodic time modulation of the wave intensity, with a typical modulation period on the order of minutes. We present results of a survey of QP emissions observed by the Wide-Band Data (WBD) instruments on board the Cluster spacecraft. All WBD data measured in the appropriate frequency range during the first 10 years of operation (2001–2010) at radial distances lower than 10 RE were visually inspected for the presence of QP emissions, resulting in 21 positively identified events. These are systematically analyzed, and their frequency ranges and modulation periods are determined. Moreover, a detailed wave analysis has been done for the events that were strong enough to be seen in low-resolution Spatio-Temporal Analysis of Field Fluctuations-Spectrum Analyzer data. Wave vectors are found to be nearly field-aligned in the equatorial region, but they become oblique at larger geomagnetic latitudes. This is consistent with a hypothesis of unducted propagation. ULF magnetic field pulsations were detected at the same time as QP emissions in 4 out of the 21 events. They were polarized in the plane perpendicular to the ambient magnetic field, and their frequencies roughly corresponded to the modulation period of the QP events.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2014
Počet záznamů: 1  

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