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”

Analysis of the Instability Growth Rate During the Jet - Background Interaction in the Magnetic Field

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21230%2F13%3A00202256" target="_blank" >RIV/68407700:21230/13:00202256 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/1674-4527/13/6/008" target="_blank" >http://dx.doi.org/10.1088/1674-4527/13/6/008</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/1674-4527/13/6/008" target="_blank" >10.1088/1674-4527/13/6/008</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Analysis of the Instability Growth Rate During the Jet - Background Interaction in the Magnetic Field

  • Original language description

    The two-stream instability is the common instability, which is responsible for many observed phenomena in nature, especially the interaction of the jets of various origin with the background plasma (e.g. extragalactic jet penetrating into the cosmic background). The dispersion relation without magnetic field is described by the well-known Buneman relation, but in 2011 Bohata, Bren, and Kulhanek derived the relation for the two-stream instability without the cold limit and with the general orientation ofmagnetic field. The maximum value of the imaginary part of the individual dispersion branches is very interesting from the physical point of view. It represents the instability growth rate which is responsible for the turbulence mode onset and subsequent reconnection on the ion radius scale accompanied by strong plasma thermalization. The paper presented here is focused on the instability growth rate dependence on various input parameters, such as magnitude and direction of magnetic fie

  • Czech name

  • Czech description

Classification

  • Type

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

  • CEP classification

    BL - Plasma physics and discharge through gases

  • OECD FORD branch

Result continuities

  • Project

  • Continuities

    S - Specificky vyzkum na vysokych skolach

Others

  • Publication year

    2013

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Research in Astronomy and Astrophysics

  • ISSN

    1674-4527

  • e-ISSN

  • Volume of the periodical

    13

  • Issue of the periodical within the volume

    6

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    8

  • Pages from-to

    687-694

  • UT code for WoS article

    000319704300008

  • EID of the result in the Scopus database