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How do fits of simulated magnetic clouds correspond to their real shapes in 3D?

SYSNO ASEP	0348472
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	How do fits of simulated magnetic clouds correspond to their real shapes in 3D?
Author(s)	Vandas, Marek (ASU-R)_{RID, ORCID} Romashets, E. P. (US) Geranios, A. (GR)
Number of authors	3
Source Title	Annales Geophysicae. - : Copernicus - ISSN 0992-7689 Roč. 28, č. 8 (2010), s. 1581-1588
Number of pages	8 s.
Action	STEREO-3/SOHO-22 Workshop: Three Eyes on the Sun, Multi-spacecraft studies of the corona and impacts on the heliosphere
Event date	27.04.2009-01.05.2009
VEvent location	Bournemouth
Country	GB - United Kingdom
Event type	WRD
Language	eng - English
Country	DE - Germany
Keywords	interplanetary magnetic fields ; magnetic clouds ; numerical simulations
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	GA205/09/0170 GA ČR - Czech Science Foundation (CSF)
	ME09032 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000281432700012
DOI	10.5194/angeo-28-1581-2010
Annotation	MHD simulations of magnetic cloud propagation are used to check our fitting procedure. Simulated spacecraft measurements are fitted by models of magnetic clouds and resulting parameters are compared with real shapes of magnetic clouds which can be directly obtained from our simulations. The comparison shows that cloud parameters are determined quite reliably for spacecraft crossings near the cloud axis.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2011

Number of the records: 1