Solar Wind Turbulence from MHD to Sub-ion Scales: High-resolution Hybrid Simulations

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00445264" target="_blank" >RIV/67985815:_____/15:00445264 - isvavai.cz</a>

Result on the web

<a href="http://dx.doi.org/10.1088/2041-8205/804/2/L39" target="_blank" >http://dx.doi.org/10.1088/2041-8205/804/2/L39</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1088/2041-8205/804/2/L39" target="_blank" >10.1088/2041-8205/804/2/L39</a>

Result language

angličtina

Original language name

Solar Wind Turbulence from MHD to Sub-ion Scales: High-resolution Hybrid Simulations

Original language description

We present results from a high-resolution and large-scale hybrid (fluid electrons and particle-in-cell protons) twodimensional numerical simulation of decaying turbulence. Two distinct spectral regions (separated by a smooth break at proton scales) develop with clear power-law scaling, each one occupying about a decade in wavenumbers.

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BN - Astronomy and celestial mechanics, astrophysics

OECD FORD branch

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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

Publication year

2015

Confidentiality

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

Name of the periodical

Astrophysical Journal Letters

ISSN

2041-8205

e-ISSN

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Volume of the periodical

804

Issue of the periodical within the volume

2

Country of publishing house

US - UNITED STATES

Number of pages

5

Pages from-to

"L39/1"-"L39/5"

UT code for WoS article

000354293200013

EID of the result in the Scopus database

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