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”

Generation mechanism of the whistler-mode waves in the plasma sheet prior to magnetic reconnection

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10191862" target="_blank" >RIV/00216208:11320/13:10191862 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/13:00423090

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.asr.2013.02.016" target="_blank" >http://dx.doi.org/10.1016/j.asr.2013.02.016</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.asr.2013.02.016" target="_blank" >10.1016/j.asr.2013.02.016</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Generation mechanism of the whistler-mode waves in the plasma sheet prior to magnetic reconnection

  • Original language description

    The whistler-mode waves and electron temperature anisotropy play a key role prior to and during magnetic reconnection. On August 21, 2002, the Cluster spacecrafts encountered a quasi-collisionless magnetic reconnection event when they crossed the plasmasheet. Prior to the southward turning of magnetospheric magnetic field and high speed ion flow, the whistler-mode waves and positive electron temperature anisotropy are simultaneously observed. Theoretic analysis shows that the electrons with positive temperature anisotropy can excite the whistler-mode waves via cyclotron resonances. Using the data of particles and magnetic field, we estimated the whistler-mode wave growth rate and the ratio of whistler-mode growth rate to wave frequency. They are 0.0016f(ce) (Electron cyclotron frequency) and 0.0086f(ce), respectively. Therefore the whistler-mode waves can grow quickly in the current sheet. The combined observations of energetic electron beams and waves show that after the southward tu

  • 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

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

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

    Advances in Space Research

  • ISSN

    0273-1177

  • e-ISSN

  • Volume of the periodical

    52

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    6

  • Pages from-to

    205-210

  • UT code for WoS article

    000320639100019

  • EID of the result in the Scopus database