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Regular variations of 3 GHz radio flux and current-loop coalescence model of solar flares.

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F03%3A01030068" target="_blank" >RIV/67985815:_____/03:01030068 - isvavai.cz</a>

  • Result on the web

  • DOI - Digital Object Identifier

Alternative languages

  • Result language

    angličtina

  • Original language name

    Regular variations of 3 GHz radio flux and current-loop coalescence model of solar flares.

  • Original language description

    The 3 GHz radio flux records of two solar flares (April 7, 1997 and March 29, 2001) with regular variations are presented. The authors interpret the observed phenomena using the current loop coalescence model of solar flares.

  • Czech name

  • Czech description

Classification

  • Type

    D - Article in proceedings

  • 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

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Others

  • Publication year

    2003

  • Confidentiality

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

Data specific for result type

  • Article name in the collection

    Solar variability as an input to the Earth's environment.

  • ISBN

  • ISSN

  • e-ISSN

  • Number of pages

    4

  • Pages from-to

    499-502

  • Publisher name

    ESA Publication division

  • Place of publication

    Noordwijk

  • Event location

    Tatranská Lomnica [SK]

  • Event date

    Jun 23, 2003

  • Type of event by nationality

    WRD - Celosvětová akce

  • UT code for WoS article