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Coronal Plasmoid Dynamics

Published online by Cambridge University Press:  12 April 2016

C. Delannée ,
S. Koutchmy ,
A. Zhukov  and
I. Veselovsky
C. Delannée
Affiliation:
Institut d’Astrophysique de Paris, CNRS, 98 bis, bd Arago, 75014 Paris, France
S. Koutchmy
Affiliation:
Institut d’Astrophysique de Paris, CNRS, 98 bis, bd Arago, 75014 Paris, France
A. Zhukov
Affiliation:
Institute of Nuclear Physics, Moscow State University, Moscow 119899, Russia
I. Veselovsky
Affiliation:
Institute of Nuclear Physics, Moscow State University, Moscow 119899, Russia

Abstract

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A possible acceleration mechanism by the magnetic force is suggested for a plasmoid, modeled as a spherical body with a magnetic dipole situated in its center of mass. The governing equations of the motion of a dipole in an inhomogeneous magnetic field are solved analytically and numerically. Both methods show the possibility for the plasmoid to be accelerated in the direction of the external field gradient.

Type
Birth and Death of Filaments
Information
International Astronomical Union Colloquium , Volume 167: New Perspectives on Solar Prominences , 1998 , pp. 388 - 392
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

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