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

Домашня сторінка
→
Фізико-технічні та математичні науки
→
Відділення фізики і астрономії
→
Кинематика и физика небесных тел
→
Кинематика и физика небесных тел, 2005 (том 21)
→
Кинематика и физика небесных тел, 2005, № 5-додаток
→
Переглянути статтю

dc.contributor.author	Konovalenko, A.A.
dc.contributor.author	Stanislavsky, A.A.
dc.contributor.author	Abranin, E.P.
dc.contributor.author	Dorovsky, V.V.
dc.contributor.author	Mel'nik, V.N.
dc.date.accessioned	2015-04-03T15:16:53Z
dc.date.available	2015-04-03T15:16:53Z
dc.date.issued	2005
dc.identifier.citation	Absorption 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.issn	0233-7665
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/79608
dc.description.abstract	We 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.sponsorship	The work was supported by the INTAS call 2003.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Кинематика и физика небесных тел
dc.subject	MS1: Decameter Radioastronomy	uk_UA
dc.title	Absorption burst in the solar sporadic radio emission at 10−30 MHz frequencies	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA