On the Stability of Siphon Flows Confined in Coronal Loops

被引:0
作者
Rita Betta
Salvatore Orlando
Giovanni Peres
Salvatore Serio
机构
[1] Osservatorio Astronomico,ESA Solar System Division, Space Science Dept.
[2] ESTEC (SO),Dipartimento di Scienze Fisiche e Astronomiche, Sezione di Astronomia
[3] Università di Palermo,undefined
来源
Space Science Reviews | 1999年 / 87卷
关键词
Mach Number; Coronal Loop; Transient Phase; Loop Length; Heat Deposition;
D O I
暂无
中图分类号
学科分类号
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:3
相关论文
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