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Determining the full halo coronal mass ejection characteristics

Published online by Cambridge University Press:  01 September 2008

V. G. Fainshtein
V. G. Fainshtein*
Affiliation:
Institute of solar-terrestrial physics SB RAS, P.O. Box 291, 664033, Irkutsk, Russia email: vfain@iszf.irk.ru
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Abstract

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In this paper we determined the parameters of 45 full halo coronal mass ejections (HCMEs) for various modifications of their cone forms (“ice cream cone models”). We show that the CME determined characteristics depend significantly on the CME chosen form. We show that, regardless of the CME chosen form, the trajectory of practically all the considered HCMEs deviate from the radial direction to the Sun-to-Earth axis at the initial stage of their movement.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 279 - 281
Copyright
Copyright © International Astronomical Union 2009

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