Počet záznamů: 1  

Electromagnetic ion cyclotron waves in the helium branch induced by multiple electromagnetic ion cyclotron triggered emissions

  1. 1.
    SYSNO ASEP0367472
    Druh ASEPJ - Článek v odborném periodiku
    Zařazení RIVJ - Článek v odborném periodiku
    Poddruh JČlánek ve WOS
    NázevElectromagnetic ion cyclotron waves in the helium branch induced by multiple electromagnetic ion cyclotron triggered emissions
    Tvůrce(i) Shoji, M. (JP)
    Omura, Y. (JP)
    Grison, Benjamin (UFA-U) RID, ORCID
    Pickett, J. (US)
    Dandouras, I. (FR)
    Engebretson, M. (US)
    Zdroj.dok.Geophysical Research Letters. - : Wiley - ISSN 0094-8276
    Roč. 38, - (2011), L17102/1-L17102/5
    Poč.str.5 s.
    Jazyk dok.eng - angličtina
    Země vyd.US - Spojené státy americké
    Klíč. slova1-2 MAGNETIC PULSATIONS ; EQUATORIAL MAGNETOSPHERE ; DISTRIBUTIONS ; STORMS
    Vědní obor RIVBL - Fyzika plazmatu a výboje v plynech
    CEPGPP209/11/P848 GA ČR - Grantová agentura ČR
    CEZAV0Z30420517 - UFA-U, BC-A (2005-2011)
    UT WOS000294620200003
    DOI10.1029/2011GL048427
    AnotaceElectromagnetic ion cyclotron (EMIC) triggered emissions with rising tones between the H(+) and He(+) cyclotron frequencies were found in the inner magnetosphere by the recent Cluster observations. Another type of EMIC wave with a constant frequency is occasionally observed below the He(+) cyclotron frequency after the multiple EMIC triggered emissions. We performed a self-consistent hybrid simulation with a one-dimensional cylindrical magnetic flux model approximating the dipole magnetic field of the Earth's inner magnetosphere. In the presence of energetic protons with a sufficient density and temperature anisotropy, multiple EMIC triggered emissions are reproduced due to the nonlinear wave growth mechanism of rising-tone chorus emissions, and a constant frequency wave in the He(+) EMIC branch is subsequently generated. Through interaction with the multiple EMIC rising-tone emissions, the velocity distribution function of the energetic protons is strongly modified.
    PracovištěÚstav fyziky atmosféry
    KontaktKateřina Adamovičová, adamovicova@ufa.cas.cz, Tel.: 272 016 012 ; Kateřina Potužníková, kaca@ufa.cas.cz, Tel.: 272 016 019
    Rok sběru2012
    Elektronická adresahttp://www.agu.org/pubs/crossref/2011/2011GL048427.shtml
Počet záznamů: 1  

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