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Statistical Moments of Active-Region Images During Solar Flares

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00399766" target="_blank" >RIV/67985815:_____/14:00399766 - isvavai.cz</a>

  • Alternative codes found

    RIV/67985556:_____/14:00399766

  • Result on the web

    <a href="http://dx.doi.org/10.1007/s11207-013-0334-4" target="_blank" >http://dx.doi.org/10.1007/s11207-013-0334-4</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1007/s11207-013-0334-4" target="_blank" >10.1007/s11207-013-0334-4</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Statistical Moments of Active-Region Images During Solar Flares

  • Original language description

    We present new temporal-evolution diagnostics of solar flares. The high-order statistical moments (skewness and kurtosis) of the H? images of active regions during solar flares were computed from their initial phases up to their maxima. The same method was used for quiet active regions for tests and comparison. We found that temporal profiles of the H? statistical moments during flares roughly correspond to those observed in soft X-rays by the GOES satellite. Maxima of the cross-correlation coefficientsbetween the skewness and the GOES X-rays were found to be 0.82???0.98, and the GOES X-rays are delayed 0???144 seconds against the skewness. We recognized that these moments are very sensitive to pre-flare activities. Therefore we used them to determinethe flare starting-time and to study the pre-flare quasi-periodic processes. We determined the periods of these pre-flare processes in an interval of 20???400 seconds by using special convolution filters and Fourier analysis. We propose

  • 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

    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

    2014

  • 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

    289

  • Issue of the periodical within the volume

    1

  • Country of publishing house

    NL - THE KINGDOM OF THE NETHERLANDS

  • Number of pages

    17

  • Pages from-to

    193-209

  • UT code for WoS article

    000327094700013

  • EID of the result in the Scopus database