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”

Fluctuation analysis of solar radio bursts associated with geoeffective X-class flares

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F11%3A00373242" target="_blank" >RIV/67985815:_____/11:00373242 - isvavai.cz</a>

  • Result on the web

    <a href="http://dx.doi.org/10.1016/j.jastp.2010.09.030" target="_blank" >http://dx.doi.org/10.1016/j.jastp.2010.09.030</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1016/j.jastp.2010.09.030" target="_blank" >10.1016/j.jastp.2010.09.030</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Fluctuation analysis of solar radio bursts associated with geoeffective X-class flares

  • Original language description

    High temporal resolution solar observations in the decimetric range (1-3 GHz) can provide additional information on solar active regions dynamics and thus contribute to better understanding of solar geoeffective events as flares and coronal mass ejections. The June 6, 2000 flares are a set of remarkable geoeffective eruptive phenomena observed as solar radio bursts (SRB) by means of the 3 GHz Ondrejov Observatory radiometer. We have selected and analyzed, applying detrended fluctuation analysis (DFA), three decimetric bursts associated to X1.1, X1.2 and X2.3 flare-classes, respectively. The association with geomagnetic activity is also reported. DFA method is performed in the framework of a radio burst automatic monitoring system. Our results may characterize the SRB evolution, computing the DFA scaling exponent, scanning the SRB time series by a short windowing before the extreme event. For the first time, the importance of DFA in the context of SRB monitoring analysis is presented.

  • 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

  • Continuities

    Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2011

  • 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 Atmospheric and Solar-Terrestrial Physics

  • ISSN

    1364-6826

  • e-ISSN

  • Volume of the periodical

    73

  • Issue of the periodical within the volume

    11

  • Country of publishing house

    GB - UNITED KINGDOM

  • Number of pages

    6

  • Pages from-to

    1311-1316

  • UT code for WoS article

    000294093500004

  • EID of the result in the Scopus database