论文标题
来自等离子体聚焦设施模拟的年轻星星的喷气机的内部结构
Internal Structure of the Jets from Young Stars Simulated at Plasma Focus Facilities
论文作者
论文摘要
在等离子体聚焦设施已有多年的年轻恒星的喷气机的实验室模拟，可以详细研究射流与周围等离子体的相互作用期间出现的活动区域的内部结构。我们发现了一种新的宽类溶液，用于理想的磁流体动力学方程，描述了显然在活性区域中实现的封闭轴对称固定流。这种流可以很好地重现在天体物理喷气机实验室模拟中观察到的血浆结构的内部结构。
The laboratory simulations of jets from young stars that have been carried out for many years at plasma focus facilities allow the internal structure of the active regions emerging during the interaction of the jet with the surrounding plasma to be studied in detail. We have found a new wide class of solutions for the equations of ideal magnetohydrodynamics describing the closed axisymmetric stationary flows that are apparently realized in the active regions. Such flows are shown to well reproduce the internal structure of the plasma structures observed in laboratory simulations of astrophysical jets.
