磁场辅助流化:一个修正的Richardson-Zaki方程

Jose Manuel Valverde, Antonio Castellanos
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引用次数: 15

摘要

通过将气体流动与外部施加的磁场耦合,磁性颗粒可以均匀流化。由磁场产生的粒子间力导致粒子聚集成链状结构,优先沿磁场线取向。在本文中,我们研究了这些特殊类型聚集体的形成对经验Richardson-Zaki (RZ)方程的影响,该方程最初是用来描述非聚集颗粒的流化床膨胀的。我们已经解决了两个重要的问题,即流动状态,这是聚集体大小的函数,以及链状聚集体的形状和方向对气体流动对流体阻力的影响。我们提出了一个修正的RZ方程(MRZE),其中由单个聚集体的终端沉降速度给出的速度尺度和RZ指数作为链长度的函数预先确定。链长取决于磁能与引力能的比值,并由磁场强度、粒子磁化强度、大小和密度来估计。我们成功地将MRZE的预测结果与已发表的关于在外加磁场存在下磁粒子膨胀的文献进行了比较。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Magnetic field assisted fluidization: A modified Richardson–Zaki equation

Magnetic particles can be uniformly fluidized by coupling the gas flow with an externally imposed magnetic field. Interparticle forces generated by the magnetic field cause aggregation of the particles in chain-like structures preferentially oriented along the magnetic field lines. In the present paper, we study the implications of the formation of these special types of aggregates on the empirical Richardson–Zaki (RZ) equation, originally proposed to describe the expansion of fluidized beds of non-aggregated particles. We have addressed two important issues, namely the flow regime, which is a function of the size of the aggregates, and the effect of shape and orientation of the chain-like aggregates with respect to gas flow on fluid drag. We propose a modified RZ equation (MRZE) in which the velocity scale, given by the terminal settling velocity of the individual aggregates, and the RZ exponent are predetermined as a function of the chain length. The chain length depends on the ratio of the magnetic energy to gravitational energy, and is estimated from the magnetic field intensity, and particle magnetization, size and density. Predictions of the MRZE are successfully compared with published results in the literature on the expansion of magnetic particles in the presence of externally applied magnetic fields.

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