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Plasma Turbulence and Kinetic Instabilities at Ion Scales in the Expanding Solar Wind

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00452203" target="_blank" >RIV/67985815:_____/15:00452203 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/15:00451773

  • Result on the web

    <a href="http://dx.doi.org/10.1088/2041-8205/811/2/L32" target="_blank" >http://dx.doi.org/10.1088/2041-8205/811/2/L32</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/2041-8205/811/2/L32" target="_blank" >10.1088/2041-8205/811/2/L32</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Plasma Turbulence and Kinetic Instabilities at Ion Scales in the Expanding Solar Wind

  • Original language description

    The relationship between a decaying strong turbulence and kinetic instabilities in a slowly expanding plasma is investigated using two-dimensional (2D) hybrid expanding box simulations. We impose an initial ambient magnetic field perpendicular to the simulation box, and we start with a spectrum of large-scale, linearly polarized, random-phase Alfvenic fluctuations that have energy equipartition between kinetic and magnetic fluctuations and vanishing correlation between the two fields. A turbulent cascade rapidly develops; magnetic field fluctuations exhibit a power-law spectrum at large scales and a steeper spectrum at ion scales. The turbulent cascade leads to an overall anisotropic proton heating, protons are heated in the perpendicular direction, and, initially, also in the parallel direction. The imposed expansion leads to generation of a large parallel proton temperature anisotropy which is at later stages partly reduced by turbulence. The turbulent heating is not sufficient to ov

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GA15-10057S" target="_blank" >GA15-10057S: Solar wind ions: correlations, constraints, and causality</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2015

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    Astrophysical Journal Letters

  • ISSN

    2041-8205

  • e-ISSN

  • Volume of the periodical

    812

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    6

  • Pages from-to

    "L32/1"-"L32/6"

  • UT code for WoS article

    000364478600018

  • EID of the result in the Scopus database