Magnetofluid Coupling: Eruptive Events in the Solar Corona
Magnetofluid Coupling: Eruptive Events in the Solar Corona
复制标题
磁流体耦合：日冕的喷发事件
DOI：
--
复制
发表时间：
2001
期刊：
影响因子：
--
通讯作者：
S. Mahajan
中科院分区：
文献类型：
--
作者：
S. Ohsaki;N. Shatashvili;Z. Yoshida;S. Mahajan
通过模拟日冕结构的“缓慢”演变的磁流体平衡态（双贝尔特拉米状态）的相互作用的磁场和速度场，原始状态的灾难性转变的条件。结果表明，在过渡，大部分的原始状态的磁能被转换为流动动能。
By modeling the coronal structures by "slowly" evolving magnetofluid equilibrium states (double Beltrami states) created by the interaction of the magnetic and velocity fields, the conditions for catastrophic transformations of the original state are derived. It is shown that, at the transition, much of the magnetic energy of the original state is converted to the flow kinetic energy.