Hostname: page-component-745bb68f8f-5r2nc Total loading time: 0 Render date: 2025-01-25T20:55:40.087Z Has data issue: false hasContentIssue false
  • English
  • Français

Stability of a Massive Current Sheet Supported by a Two-Dimensional Potential Magnetic Field

Published online by Cambridge University Press:  19 July 2016

J.J. Aly  and
S. Colombi
J.J. Aly
Affiliation:
Service d'Astrophysique Centre d'Etudes Nucléaires de Saclay 91191 Gif-sur-Yvette Cedex France
S. Colombi
Affiliation:
Service d'Astrophysique Centre d'Etudes Nucléaires de Saclay 91191 Gif-sur-Yvette Cedex France

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.

Necessary and sufficient criteria of linear ideal magnetohydrodynamic stability are derived for a massive current sheet - idealizing a solar prominence - supported against gravity by a two-dimensional potential magnetic field.

Type
VII. Magnetic Reconnection and Coronal Evolution
Information
Symposium - International Astronomical Union , Volume 142: Basic Plasma Processes on the Sun , 1990 , pp. 341 - 342
Copyright
Copyright © Kluwer 1990 

References

REFERENCES

Anzer, U. (1969). “Stability analysis of the Kippenhahn - Schlüter model of solar filaments”, Solar Phys. 108, 26.Google Scholar
Anzer, U. (1989). “Structure and equilibrium of prominences”, in Priest, E.R. (ed.), Dynamics and Structure of Quiescent Solar Prominences, Kluwer Academic Publishers, Dordrecht, p. 143.Google Scholar