Magnetic Field Turbulence in the Solar Wind at Sub-ion Scales: In Situ Observations and Numerical Simulations

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00538193" target="_blank" >RIV/67985815:_____/20:00538193 - isvavai.cz</a>

Result on the web

<a href="http://hdl.handle.net/11104/0316013" target="_blank" >http://hdl.handle.net/11104/0316013</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3389/fspas.2020.563075" target="_blank" >10.3389/fspas.2020.563075</a>

Result language

angličtina

Original language name

Magnetic Field Turbulence in the Solar Wind at Sub-ion Scales: In Situ Observations and Numerical Simulations

Original language description

We investigate the transition of the solar wind turbulent cascade from MHD to sub-ion range by means of a detailed comparison between in situ observations and hybrid numerical simulations. In particular, we focus on the properties of the magnetic field and its component anisotropy in Cluster measurements and hybrid 2D simulations.

Czech name

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Czech description

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Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

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OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

<a href="/en/project/GA18-08861S" target="_blank" >GA18-08861S: Plasma turbulence at ion scales in the solar wind</a><br>

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2020

Confidentiality

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

Name of the periodical

Frontiers in Astronomy and Space Sciences

ISSN

2296-987X

e-ISSN

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Volume of the periodical

7

Issue of the periodical within the volume

December

Country of publishing house

CH - SWITZERLAND

Number of pages

15

Pages from-to

563075

UT code for WoS article

000603079700001

EID of the result in the Scopus database

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