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
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Czech description
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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
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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
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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
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