- Proton heating by pick-up ion driven cyclotron waves in the outer hel…
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Proton heating by pick-up ion driven cyclotron waves in the outer heliosphere: Hybrid expanding box simulations

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    SYSNO ASEP0472216
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleProton heating by pick-up ion driven cyclotron waves in the outer heliosphere: Hybrid expanding box simulations
    Author(s) Hellinger, Petr (UFA-U) RID, ORCID
    Trávníček, P. M. (CZ)
    Number of authors2
    Article number32
    Source TitleAstrophysical Journal - ISSN 0004-637X
    Roč. 832, č. 1 (2016)
    Number of pages7 s.
    Languageeng - English
    CountryUS - United States
    Keywordssolar wind ; instabilities ; plasmas
    Subject RIVBL - Plasma and Gas Discharge Physics
    OECD categoryFluids and plasma physics (including surface physics)
    Institutional supportUFA-U - RVO:68378289
    UT WOS000388603600014
    EID SCOPUS84996490263
    DOI https://doi.org/10.3847/0004-637X/832/1/32
    AnnotationUsing a one-dimensional hybrid expanding box model, we investigate properties of the solar wind in the outer heliosphere. We assume a proton-electron plasma with a strictly transverse ambient magnetic field and, aside from the expansion, we take into account the influence of a continuous injection of cold pick-up protons through the charge-exchange process between the solar wind protons and hydrogen of interstellar origin. The injected cold pick-up protons form a ring distribution function, which rapidly becomes unstable, and generate Alfven cyclotron waves. The Alfvwn cyclotron waves scatter pick-up protons to a spherical shell distribution function that thickens over that time owing to the expansion-driven cooling. The Alfvwn cyclotron waves heat solar wind protons in the perpendicular direction (with respect to the ambient magnetic field) through cyclotron resonance. At later times, the Alfven cyclotron waves become parametrically unstable and the generated ion-acoustic waves heat protons in the parallel direction through Landau resonance. The resulting heating of the solar wind protons is efficient on the expansion timescale.
    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 Publishing2017
Number of the records: 1  

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