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Whistler-mode waves inside flux pileup region: Structured or unstructured?

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F14%3A10289787" target="_blank" >RIV/00216208:11320/14:10289787 - isvavai.cz</a>

  • Alternative codes found

    RIV/68378289:_____/14:00441007

  • Result on the web

    <a href="http://dx.doi.org/10.1002/2014JA020204" target="_blank" >http://dx.doi.org/10.1002/2014JA020204</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1002/2014JA020204" target="_blank" >10.1002/2014JA020204</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Whistler-mode waves inside flux pileup region: Structured or unstructured?

  • Original language description

    During reconnection, a flux pileup region (FPR) is formed behind a dipolarization front in an outflow jet. Inside the FPR, the magnetic field magnitude and Bz component increase and the whistler-mode waves are observed frequently. As the FPR convects toward the Earth during substorms, it is obstructed by the dipolar geomagnetic field to form a near-Earth FPR. Unlike the structureless emissions inside the tail FPR, we find that the whistler-mode waves inside the near-Earth FPR can exhibit a discrete structure similar to chorus. Both upper band and lower band chorus are observed, with the upper band having a larger propagation angle (and smaller wave amplitude) than the lower band. Most chorus elements we observed are rising-tone type, but some are falling-tone type. We notice that the rising-tone chorus can evolve into falling-tone chorus within <3s. One of the factors that may explain why the waves are unstructured inside the tail FPR but become discrete inside the near-Earth FPR is th

  • 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

    <a href="/en/project/7E12026" target="_blank" >7E12026: Monitoring, Analyzing and Assessing Radiation Belt Loss and Energization</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2014

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Journal of Geophysical Research - Space Physics

  • ISSN

    2169-9380

  • e-ISSN

  • Volume of the periodical

    119

  • Issue of the periodical within the volume

    11

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    12

  • Pages from-to

    9089-9100

  • UT code for WoS article

    000346792100026

  • EID of the result in the Scopus database