Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-25T03:42:44.337Z Has data issue: false hasContentIssue false
  • English
  • Français

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: [email protected]
D. Odstrcil
Affiliation:
University of Colorado/CIRES and NOAA/Space Environment Center, Boulder, CO 80305, USA email: [email protected]
S. Watari
Affiliation:
National Institute of Information and Communications Technology, 4-2-1 Nukuikita, Koganei, Tokyo 184-8795, Japan email: [email protected]
A. Geranios
Affiliation:
Physics Department, University of Athens, Panepistimioupoli-Kouponia, Athens 15771, Greece email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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