All

What are you looking for?

All
Projects
Results
Organizations

Quick search

  • Projects supported by TA ČR
  • Excellent projects
  • Projects with the highest public support
  • Current projects

Smart search

  • That is how I find a specific +word
  • That is how I leave the -word out of the results
  • “That is how I can find the whole phrase”

Three-dimensional simulations of solar wind turbulence with the hybrid code CAMELIA

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00500549" target="_blank" >RIV/67985815:_____/18:00500549 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/1742-6596/1031/1/012002" target="_blank" >http://dx.doi.org/10.1088/1742-6596/1031/1/012002</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1742-6596/1031/1/012002" target="_blank" >10.1088/1742-6596/1031/1/012002</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Three-dimensional simulations of solar wind turbulence with the hybrid code CAMELIA

  • Original language description

    We investigate the spectral properties of plasma turbulence from fluid to sub-ion scales by means of high-resolution three-dimensional (3D) numerical simulations performed with the hybrid particle-in-cell (HPIC) code CAMELIA. We produce extended turbulent spectra with well-defined power laws for the magnetic, ion bulk velocity, density, and electric fluctuations. The present results are in good agreement with previous two-dimensional (2D) HPIC simulations, especially in the kinetic range of scales, and reproduce several features observed in solar wind spectra. By providing scaling tests on many different architectures and convergence studies, we prove CAMELIA to represent a very efficient, accurate and reliable tool for investigating the development of the turbulent cascade in the solar wind, being able to cover simultaneously several decades in wavenumber, also in 3D.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

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

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2018

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Proceedings of the 12th International Conference on Numerical Modeling of Space Plasma Flows: ASTRONUM 2017

  • ISBN

  • ISSN

    1742-6588

  • e-ISSN

  • Number of pages

    13

  • Pages from-to

  • Publisher name

    Institute of Physics Publishing

  • Place of publication

    Bristol

  • Event location

    Saint-Malo

  • Event date

    Jun 26, 2017

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article

    000454784100002