Kelvin-Helmholtz instability and resonant flow instability in a 1-dimensional coronal plume model
作者:
J. Andries,
M. Goossens,
期刊:
AIP Conference Proceedings
(AIP Available online 1900)
卷期:
Volume 537,
issue 1
页码: 136-143
ISSN:0094-243X
年代: 1900
DOI:10.1063/1.1324933
出版商: AIP
数据来源: AIP
摘要:
In a previous paper we have illustrated the concept of resonant flow instability of the trapped modes both in a 1-D slab model and a 1-D cylindrical model for a coronal plume in a cold plasma. We found that much larger values of the velocity shear are needed for Kelvin-Helmholtz than for resonant instability to occur. The aim of this paper is to study the effect of a non-zero plasma pressure on the eigenmodes of the plume structure. We show that the instability most probably to occur in coronal plumes is due to the resonant coupling of slow body modes to local resonant Alfve´n waves. These instabilities could lead to disruption of the coronal plumes and to the mixing with interplume plasma. ©2000 American Institute of Physics.
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