On the stability of siphon flows confined in coronal loops

被引:2
作者
Betta, R
Orlando, S
Peres, G
Serio, S
机构
[1] Osservatorio Astron, I-90134 Palermo, Italy
[2] European Space Agcy, Dept Space Sci, Solar Syst Div, ESTEC SO, NL-2200 AG Noordwijk, Netherlands
[3] Univ Palermo, Dipartimento Sci Fis & Astron, Sez Astron, I-90134 Palermo, Italy
关键词
D O I
10.1023/A:1005182503751
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use a time-dependent hydrodynamic model to study the dynamics of siphon flows triggered by differences of pressure or heat deposition asymmetries between the two footpoints of a coronal loop. We show that steady pressure driven flows in a uniformly heated loop are unstable, whereas those driven by asymmetries in the heating function may be stable. We also show that, in these cases, relatively cool loops might be filled far above their static pressure scale height.
引用
收藏
页码:133 / 136
页数:4
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