Absorption burst in the solar sporadic radio emission at 10−30 MHz frequencies

dc.contributor.authorKonovalenko, A.A.
dc.contributor.authorStanislavsky, A.A.
dc.contributor.authorAbranin, E.P.
dc.contributor.authorDorovsky, V.V.
dc.contributor.authorMel'nik, V.N.
dc.date.accessioned2015-04-03T15:16:53Z
dc.date.available2015-04-03T15:16:53Z
dc.date.issued2005
dc.description.abstractWe report the results of UTR-2 radio telescope observations of an absorption burst at the decameter range. This event is associated with two consecutive M-class flares and happened after the second M-flare. The latter flare was accompanied by Type II, Type IV radio sweeps and a CME. The observed bandwidth of the burst is about 20 MHz. The size of the absorption region is compared with the solar radius. The frequency drift rate of the absorption burst is about −0.12 MHz/s. The features of this event are discussed.uk_UA
dc.description.sponsorshipThe work was supported by the INTAS call 2003.uk_UA
dc.identifier.citationAbsorption burst in the solar sporadic radio emission at 10−30 MHz frequencies / A.A. Konovalenko, A.A. Stanislavsky, E.P. Abranin, V.V. Dorovsky, V.N. Mel'nik // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 78-81. — Бібліогр.: 14 назв. — англ.uk_UA
dc.identifier.issn0233-7665
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/79608
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofКинематика и физика небесных тел
dc.statuspublished earlieruk_UA
dc.subjectMS1: Decameter Radioastronomyuk_UA
dc.titleAbsorption burst in the solar sporadic radio emission at 10−30 MHz frequenciesuk_UA
dc.typeArticleuk_UA

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