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Experimental study of the frosting characteristic of water on a cold surface in the magnetic field

机译:磁场冷表面磨砂特性的实验研究

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In this paper, the effect of the magnetic field on the frost formation over a cold surface was investigated on the basis of an established visualization system equipped with a magnetic field generator. Various factors such as atmosphere temperature, relative humidity, cold surface temperature, and surface wettability were considered in this study. The thickness of the frost layer, equivalent radius and the morphology of the ice crystal were observed and measured during the courses of droplet growth, freezing, and the frost growth. In order to analyze the effect of the magnetic field on frosting, the coverage fraction was proposed to evaluate the final frosting characteristics. It has been found that the coverage fraction decreases slowly with the increase of the magnetic flux density, which means that the frost formation on the cold surface in a magnetic field is less than that in a non-magnetic field. In addition, a mathematical model was proposed to describe the freezing process with a difference of less than 25% compared to the experimental data. It indicates that the magnetic field plays a significant impact on the freezing process, and the increase of the magnetic flux density leads to a small decrease in the phase change force. It takes a long freezing time for the droplet to enter a solid state, and therefore the crystal radius is small. The crystal boundary is much more regular and the thickness of the frost layer is thinner than that under a nonmagnetic condition since the hydrogen bonds of water are stronger and the configuration is more ordered and stable. Under such circumstances, a large phase change driving force is needed to overcome the magnetic force. The correlations are presented to describe the variation of the radius and thickness of ice crystal, which is beneficial to the defrosting control technology.
机译:在本文中,基于配备有磁场发生器的建立的可视化系统,研究了磁场对冷表面上霜形成的影响。在本研究中考虑了各种因素,如大气温度,相对湿度,冷表面温度和表面润湿性。在液滴生长,冷冻和霜冻生长的过程中观察和测量冰晶层,等效半径和冰晶形态的厚度。为了分析磁场对磨砂时的效果,提出了覆盖率来评估最终的磨砂特性。已经发现,随着磁通密度的增加,覆盖率分数缓慢降低,这意味着在磁场中的冷表面上的霜形成小于非磁场中的霜。此外,提出了一种数学模型来描述与实验数据相比差异小于25%的冷冻过程。它表明磁场对冷冻过程起显着影响,并且磁通密度的增加导致相变力的小降低。液滴进入固态需要长时间冻结时间,因此晶体半径很小。晶界更规则,霜层的厚度比在非磁性条件下的厚度较薄,因为水的氢键更强,并且该构造更具有序且稳定。在这种情况下,需要大相变化驱动力来克服磁力。提出了相关性以描述冰晶的半径和厚度的变化,这有利于除霜控制技术。

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