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Oscillations in the 45-5000 MHz Radio Spectrum of the 18 April 2014 Flare

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00479175" target="_blank" >RIV/67985815:_____/17:00479175 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1007/s11207-017-1117-0" target="_blank" >http://dx.doi.org/10.1007/s11207-017-1117-0</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s11207-017-1117-0" target="_blank" >10.1007/s11207-017-1117-0</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Oscillations in the 45-5000 MHz Radio Spectrum of the 18 April 2014 Flare

  • Original language description

    Using a new type of oscillation map, made from the radio spectra by the wavelet technique, we study the 18 April 2014 M7.3 flare. We find a quasi-periodic character of this flare with periods in the range 65 - 115 seconds. At the very beginning of this flare, in connection with the drifting pulsation structure (plasmoid ejection), we find that the 65 - 115 s oscillation phase slowly drifts towards lower frequencies, which indicates an upward propagating wave initiated at the start of the magnetic reconnection. Many periods (1 - 200 seconds) are found in the drifting pulsation structure, which documents multi-scale and multi-periodic processes. On this drifting structure, fiber bursts with a characteristic period of about one second are superimposed, whose frequency drift is similar to that of the drifting 65 - 115 s oscillation phase. We also checked periods found in this flare by the EUV Imaging Spectrometer (EIS)/Hinode and Interface Region Imaging Spectrograph (IRIS) observations. We recognize the type III bursts (electron beams) as proposed, but their time coincidence with the EIS and IRIS peaks is not very good. The reason probably is that the radio spectrum is a whole-disk record consisting of all bursts from any location, while the EIS and IRIS peaks are emitted only from locations of slits in the EIS and IRIS observations.

  • 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

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2017

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Solar Physics

  • ISSN

    0038-0938

  • e-ISSN

  • Volume of the periodical

    292

  • Issue of the periodical within the volume

    7

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    15

  • Pages from-to

    "94/1"-"94/15"

  • UT code for WoS article

    000406304300012

  • EID of the result in the Scopus database

    2-s2.0-85021717134