Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-13T12:26:54.454Z Has data issue: false hasContentIssue false
  • English
  • Français

Magnetic Field Configuration Around Large Flux Ropes

Published online by Cambridge University Press:  03 June 2005

E. Romashets  and
M. Vandas
E. Romashets
Affiliation:
IZMIRAN, Troitsk, 149190, Russia email: romash@izmiran.rssi.ru
M. Vandas
Affiliation:
Astronomical Institute, 14131 Praha 4, Czech Republic email: vandas@ig.cas.cz
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.

An analytical method is used to model a magnetic field distribution in the vicinity of a large interplanetary or solar flux rope. The field is a sum of the pre-existing one and an additional current-free part. An example using real data is shown.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Keywords

Sun: magnetic fieldsSun: coronal mass ejections (CMEs)methods: analytical
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUS226 , September 2004 , pp. 428 - 429
Copyright
© 2005 International Astronomical Union