Number of the records: 1

Coronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare

SYSNO ASEP	0323677
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Coronal fast wave trains of the decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare
Title	Rychlé koronální vlny decimetrického typu IV rádiového vzplanutí pozorovaného během závěrečné fáze erupce dne 6. června 2000
Author(s)	Mészárosová, Hana (ASU-R)_{RID, ORCID} Sawant, H. S. (BR) Cecatto, J.R. (BR) Rybák, J. (SK) Karlický, Marian (ASU-R)_{RID, ORCID} Fernandes, F. C. R. (BR) de Andrade, M. C. (BR) Jiřička, Karel (ASU-R)
Source Title	Advances in Space Research. - : Elsevier - ISSN 0273-1177 Roč. 43, č. 10 (2009), s. 1479-1483
Number of pages	5 s.
Language	eng - English
Country	GB - United Kingdom
Keywords	Sun ; corona ; radio radiation
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000266276100002
DOI	10.1016/j.asr.2009.01.032
Annotation	The 22 min long decimetric type IV radio event observed during the decay phase of the June 6, 2000 flare simultaneously by the Brazilian Solar Spectroscope (BSS) and the Ondrejov radiospectrograph in frequency range 1200–4500 MHz has been analyzed. We have found that the characteristic periods of about 60 s belong to the long-period spectral component of the fast wave trains with a tadpole pattern in their wavelet power spectra. We have detected these trains in the whole frequency range 1200–4500 MHz. In this paper, we focus on two examples of wave trains in a loop segment and the main statistical parameters are studied and discussed.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2010

Number of the records: 1