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Decametric radio bursts associated with the 13 July 2004 CME event at frequencies 10–30 MHz

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dc.contributor.author Boiko, A.I.
dc.contributor.author Melnik, V.N.
dc.contributor.author Konovalenko, A.A.
dc.contributor.author Abranin, E.P.
dc.contributor.author Dorovskyy, V.V.
dc.contributor.author Rucker, H.O.
dc.date.accessioned 2017-06-04T18:02:06Z
dc.date.available 2017-06-04T18:02:06Z
dc.date.issued 2012
dc.identifier.citation Decametric radio bursts associated with the 13 July 2004 CME event at frequencies 10–30 MHz / A.I. Boiko, V.N. Melnik, A.A. Konovalenko, E.P. Abranin, V.V. Dorovskyy, H.O. Rucker // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 76-78. — Бібліогр.: 9 назв. — англ. uk_UA
dc.identifier.issn 2227-1481
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119153
dc.description.abstract We report on the observations of solar type IV burst and its precursors on the 13 of July 2004 at frequencies 10 − 30 MHz. The radio telescope UTR-2 observational data compiled from SOHO, WIND, NDA, RHESSI, GOES data were used. The main properties (frequency drift rate, duration, flux) of type IV burst and its precursors, namely solar type III and type II bursts, are analysed. We consider the type IV burst connected with appearance of the coronal mass ejection, which occurrence coincides with the type IV burst beginning. Several physical characteristics of this CME were estimated. uk_UA
dc.description.sponsorship The authors are grateful to SOHO, WIND, HiRAS and Nancay teams for the open data policy. uk_UA
dc.language.iso en uk_UA
dc.publisher Головна астрономічна обсерваторія НАН України uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title Decametric radio bursts associated with the 13 July 2004 CME event at frequencies 10–30 MHz uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


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