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Zebra-stripe sources in the double-plasma resonance model of solar radio zebras

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00511433" target="_blank" >RIV/67985815:_____/19:00511433 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1051/0004-6361/201935281" target="_blank" >https://doi.org/10.1051/0004-6361/201935281</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/201935281" target="_blank" >10.1051/0004-6361/201935281</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Zebra-stripe sources in the double-plasma resonance model of solar radio zebras

  • Original language description

    The most probable model of zebras is that based on double-plasma resonance (DPR) instability. The paper wants to contribute to a verification of this model. We used analytical methods. We studied the DPR model in two scenarios: a model with the zebra-stripe sources in a single loop and a model with the zebra-stripe sources moving through a fan of magnetic field lines. In the first case, we found several new relations among the parameters of zebra stripes and their sources, which can be used to analyze observed zebras and thus to verify if the zebra is generated according to the DPR model. These relations were derived for the zebra-stripe sources distributed along the loop and also for those having some extent in the loop radius. In the scenario with the moving zebra-stripe sources, we determined the parameters of the 14 December 2006 zebra and estimated a change of the ratio of magnetic field and density scales causing the change of zebra-stripe frequencies. In this case we found that this zebra can be also explained in the model with the zebra-stripe sources in a single loop. Both the interpretations are discussed.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2019

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    1432-0746

  • e-ISSN

  • Volume of the periodical

    624

  • Issue of the periodical within the volume

    April

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    6

  • Pages from-to

    A119

  • UT code for WoS article

    000465083200001

  • EID of the result in the Scopus database

    2-s2.0-85065259154