Davidson P A, Sreenivasan Binod, Aspden A J
Department of Engineering, University of Cambridge, Cambridge, CB2 1PZ, United Kingdom.
Phys Rev E Stat Nonlin Soft Matter Phys. 2007 Feb;75(2 Pt 2):026304. doi: 10.1103/PhysRevE.75.026304. Epub 2007 Feb 6.
We investigate the evolution of localized blobs of swirling or buoyant fluid in an infinite, inviscid, electrically conducting fluid. We consider the three cases of a strong imposed magnetic field, a weak imposed magnetic field, and no magnetic field. For a swirling blob in the absence of a magnetic field, we find, in line with others, that the blob bursts radially outward under the action of the centrifugal force, forming a thin annular vortex sheet. A simple model of this process predicts that the vortex sheet thins exponentially fast and that it moves radially outward with constant velocity. These predictions are verified by high-resolution numerical simulations. When an intense magnetic field is applied, this phenomenon is suppressed, with the energy and angular momentum of the blob now diffusing axially along the magnetic field lines, converting the blob into a columnar structure. For modest or weak magnetic fields, there are elements of both types of behavior, with the radial bursting dominating over axial diffusion for weak fields. However, even when the magnetic field is very weak, the flow structure is quite distinct to that of the nonmagnetic case. In particular, a small but finite magnetic field places a lower bound on the thickness of the annular vortex sheet and produces an annulus of counter-rotating fluid that surrounds the vortex core. The behavior of the buoyant blob is similar. In the absence of a magnetic field, it rapidly develops the mushroomlike shape of a thermal, with a thin vortex sheet at the top and sides of the mushroom. Again, a simple model of this process predicts that the vortex sheet at the top of the thermal thins exponentially fast and rises with constant velocity. These predictions are consistent with earlier numerical simulations. Curiously, however, it is shown that the net vertical momentum associated with the blob increases linearly in time, despite the fact that the vertical velocity at the front of the thermal is constant. As with the swirling blob, an imposed magnetic field inhibits the formation of a vortex sheet. A strong magnetic field completely suppresses the phenomenon, replacing it with an axial diffusion of momentum, while a weak magnetic field allows the sheet to form, but places a lower bound on its thickness. The magnetic field does not, however, change the net vertical momentum of the blob, which always increases linearly with time.
我们研究了无限大、无粘性、导电流体中旋转或浮力流体的局部团块的演化。我们考虑了强外加磁场、弱外加磁场和无磁场这三种情况。对于无磁场时的旋转团块,我们与其他人的研究结果一致地发现,团块在离心力作用下径向向外破裂,形成一个薄的环形涡旋片。这个过程的一个简单模型预测,涡旋片以指数速度变薄,并以恒定速度径向向外移动。这些预测通过高分辨率数值模拟得到了验证。当施加强磁场时,这种现象受到抑制,团块的能量和角动量现在沿着磁力线轴向扩散,将团块转变为柱状结构。对于适度或弱磁场,两种行为都有体现,对于弱磁场,径向破裂比轴向扩散更占主导。然而,即使磁场非常弱,流动结构与无磁场情况也有很大不同。特别是,一个小但有限的磁场对环形涡旋片的厚度设定了下限,并产生一个围绕涡旋核心的反向旋转流体环。浮力团块的行为类似。在没有磁场的情况下,它迅速发展成热羽流的蘑菇状,在蘑菇顶部和侧面有一个薄的涡旋片。同样,这个过程的一个简单模型预测,热羽流顶部的涡旋片以指数速度变薄并以恒定速度上升。这些预测与早期的数值模拟一致。然而,奇怪的是,结果表明与团块相关的净垂直动量随时间线性增加,尽管热羽流前端的垂直速度是恒定不变的。与旋转团块一样,外加磁场会抑制涡旋片的形成。强磁场完全抑制了这种现象,取而代之的是动量的轴向扩散,而弱磁场允许涡旋片形成,但对其厚度设定了下限。然而,磁场并不会改变团块的净垂直动量,净垂直动量总是随时间线性增加。