Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-26T13:20:13.706Z Has data issue: false hasContentIssue false

On a Possible Mechanism of Quiescent Prominence Destabilization

Published online by Cambridge University Press:  12 April 2016

P. Nenovski
Affiliation:
Geophysical Institute, Acad. G. Bonchev Str, 1113 Sofia, Bulgaria
V.N. Dermendjiev
Affiliation:
Institute of Astronomy, 72 Trakia Blvd., 1784 Sofia, Bulgaria
M.S. Madjarska
Affiliation:
Institute of Astronomy, 72 Trakia Blvd., 1784 Sofia, Bulgaria
J.-C. Vial
Affiliation:
I.A.S., Université Paris XI-CNRS, Bâtiment 121, 91405 Orsay, 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.

The possibility of multiple reflections generating standing surface wave modes carrying field-aligned current (FAC) in an arch-like prominence structure is studied. The conditions for enhancement of FAC leading to observable destabilising effects are specified.

Type
Birth and Death of Filaments
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Engvold, O., Hirayama, T., Leroy, J.-L., Priest, E.R. and Tandberg-Hanssen, E. 1990, in Dynamics of Quiescent Prominences, Ruždjak, V. and Tandberg-Hanssen, E. (eds.), Springer-Verlag, New York, p. 294 Google Scholar
Madjarska, M.S., Dermendjiev, V.N., Mouradian, Z. and Nenovski, P. 1996, Astroph. Lett. and Comm, 34, 113 Google Scholar
Nenovski, P., Momchilov, G. 1987, Planet. Space Sci., 35, 1561 Google Scholar
Vernazza, J., Avrett, E., Loeser, R. 1981, ApJS, 45, 635 Google Scholar