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A Very Small and Super Strong Zebra Pattern Burst at the Beginning of a Solar Flare

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00433653" target="_blank" >RIV/67985815:_____/14:00433653 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1088/0004-637X/790/2/151" target="_blank" >http://dx.doi.org/10.1088/0004-637X/790/2/151</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1088/0004-637X/790/2/151" target="_blank" >10.1088/0004-637X/790/2/151</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    A Very Small and Super Strong Zebra Pattern Burst at the Beginning of a Solar Flare

  • Original language description

    Microwave emission with spectral zebra pattern structures (ZPs) is frequently observed in solar flares and the Crab pulsar. The previous observations show that ZP is a structure only overlapped on the underlying broadband continuum with slight incrementsand decrements. This work reports an unusually strong ZP burst occurring at the beginning of a solar flare observed simultaneously by two radio telescopes located in China and the Czech Republic and by the EUV telescope on board NASA's satellite Solar Dynamics Observatory on 2013 April 11. It is a very short and super strong explosion whose intensity exceeds several times that of the underlying flaring broadband continuum emission, lasting for just 18 s. EUV images show that the flare starts from several small flare bursting points (FBPs).

  • Czech name

  • Czech description

Classification

  • Type

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

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

Result continuities

  • Project

    <a href="/en/project/GAP209%2F12%2F0103" target="_blank" >GAP209/12/0103: Radio and X-ray diagnostics of primary-energy-release processes in solar flares and their numerical simulations</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

    Astrophysical Journal

  • ISSN

    0004-637X

  • e-ISSN

  • Volume of the periodical

    790

  • Issue of the periodical within the volume

    2

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    6

  • Pages from-to

    "151/1"-"151/6"

  • UT code for WoS article

    000339115800068

  • EID of the result in the Scopus database