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Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes

SYSNO ASEP	0355335
Document Type	C - Proceedings Paper (int. conf.)
R&D Document Type	Conference Paper
Title	Modeling of Magnetic Field Disturbances in Sheath Region of Interplanetary Magnetic Clouds of Elliptical Shapes
Author(s)	Vandas, Marek (ASU-R)_{RID, ORCID} Romashets, E. P. (US)
Source Title	Twelfth International Solar Wind Conference. Proceedings Paper. - New York : Melville, 2010 / Maksimovic M. ; Issautier K. ; Meyer-Vernet N. ; Moncuquet M. ; Pantellini F. - ISSN 0094-243X - ISBN 978-0-7354-0759-6
Pages	s. 399-402
Number of pages	4 s.
Publication form	Print - P
Action	Twelve International Solar Wind Conference
Event date	21.06.2009-26.06.2009
VEvent location	Saint-Malo
Country	FR - France
Event type	WRD
Language	eng - English
Country	US - United States
Keywords	solar magnetism ; corona ; magnetohydrodynamics
Subject RIV	BL - Plasma and Gas Discharge Physics
R&D Projects	1QS300120506 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
	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	000281438100094
DOI	10.1063/1.3395886
Annotation	It is widely accepted that magnetic disturbances around fast interplanetary magnetic clouds can play an important role in their geo-effectiveness. An analytical solution for magnetic field in the sheath region of a cylindrical magnetic cloud with an elliptical cross-section is proposed. Upstream magnetic field can have an arbitrary direction. Normal magnetic field components are conserved through the bow shock with a high accuracy.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2015

Number of the records: 1