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Impulsively Generated Wave Trains in a Solar Coronal Loop

SYSNO ASEP	0353995
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Impulsively Generated Wave Trains in a Solar Coronal Loop
Author(s)	Jelínek, P. (CZ) Karlický, Marian (ASU-R)_{RID, ORCID}
Source Title	IEEE Transactions on Plasma Science. - : Institute of Electrical and Electronics Engineers - ISSN 0093-3813 Roč. 38, č. 9 (2010), s. 2243-2248
Number of pages	6 s.
Language	eng - English
Country	US - United States
Keywords	Coronal loops ; magnetohydrodynamis ; oscillations
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	IAA300030701 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	GAP209/10/1680 GA ČR - Czech Science Foundation (CSF)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000283252500021
DOI	10.1109/TPS.2010.2052371
Annotation	Inpulsively generated fast magnetoacoustic wave trains in a solar coronal loop are numerically studied. The problem is considered as 2-D in space, and for the description, the full set of MHD equations is used. These studies are very important in connection with observations of so called tadpole structures.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2011

Number of the records: 1