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Propagation of Magnetic Clouds – MHD Simulations of Real Events

Published online by Cambridge University Press:  03 June 2005

M. Vandas ,
D. Odstrcil ,
S. Watari  and
A. Geranios
M. Vandas
Affiliation:
Astronomical Institute, 14131 Praha 4, Czech Republic email: vandas@ig.cas.cz
D. Odstrcil
Affiliation:
University of Colorado/CIRES and NOAA/Space Environment Center, Boulder, CO 80305, USA email: Dusan.Odstrcil@noaa.gov
S. Watari
Affiliation:
National Institute of Information and Communications Technology, 4-2-1 Nukuikita, Koganei, Tokyo 184-8795, Japan email: watari@nict.go.jp
A. Geranios
Affiliation:
Physics Department, University of Athens, Panepistimioupoli-Kouponia, Athens 15771, Greece email: ageran@cc.uoa.gr
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Abstract

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The paper describes our approach to simulations of real interplanetary events, consisting of four steps: (i) determination of background solar wind, (ii) parameterization of a model flux rope, (iii) launching it into the solar wind, and (iv) calculating its propagation and evolution.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: coronal mass ejections (CMEs)solar windMHD
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 430 - 432
Copyright
© 2005 International Astronomical Union