磁性流体的非线性声参量B/A的研究

报导了水基和酯基磁性流体的非线性声参量B／A值随浓度和温度的变化关系。实验研究表明，磁性流体的B／A值随磁性颗粒浓度的增大而线性增大；磁性流体的B／A值随温度的升高而线性增大。还对超声波在磁性流体中传播的声速进行了精确测量。     

磁流体SERS超灵敏检测鱼表面农药残留

将表面增强拉曼散射(SERS)光谱与磁性流体的结合应用于SERS即时(POC)检测,首先将银纳米粒子修饰到磁性Fe3O4纳米粒子表面制备磁性等离子体(AgMNPs)。AgMNPs的强磁响应性能够快速分离和检测鱼皮表面的目标分析物。制备了具有不同腔体的微流体芯片,通过磁场限制磁流体在不同腔体内的分布,从而增强了SERS信号并将检测限提高了两个数量级。磁性流体POC传感器以优异的选择性和低至皮摩尔级的高灵敏度成功检测到鱼中的孔雀石绿(MG)。实现了一种无标记、无损的光学传感方法,具有检测食品或环境中各种有害成分的潜力。     

磁性碳纳米管吸附去除水中甲基橙的研究

采用高温催化裂解法制备碳纳米管,对其用浓硝酸氧化法进行纯化处理,并用化学共沉淀方法制备了磁性碳纳米管(简称磁性管)。利用场发射扫描电子显微镜对磁性管进行了表征。将磁分离技术应用于碳纳米管吸附性能研究,探索碳纳米管负载磁性颗粒后对甲基橙的吸附性能,寻找最佳实验条件,对吸附质溶液进行紫外-可见吸收光谱分析。同时,进行了磁性管的脱附和再吸附性能研究。     

磁性流体的法拉第旋转

介绍了磁性流体拉法第旋转的形成原因，影响因素及数学模型，结果表明，磁性流本中磁性粒子磁场中成链状结构的链长度对拉法第旋转的形成起决定作用，磁场强度，磁性流体饱和磁化强度，样品池厚度，光波长及温度等都具有一定作用。     

一种可直接使用的磁性光热纳米流体

本文通过"两步法"制备了一种具有高光热转换效率的Fe304-H20磁性纳米流体。该纳米流体可以通过磁分离技术实现纳米颗粒与基液的分离,使得纳米流体基液得以直接使用,同时具有优异的可重复利用性能。实验结果表明,在1200 s内其光热转化效率高达70.2%,并且经过60次的循环使用后无明显的衰减。此研究结果为实现纳米流体基液的直接应用提供了可行性的方案。     

磁性ICF靶丸的化学镀工艺制备与表征

 采用化学镀工艺在ICF聚苯乙烯靶丸表面包覆了一层磁性的Ni-P合金镀层，并分别用扫描电子显微镜、能谱仪、X射线衍射仪以及振动样品磁强计对其形貌、组成、结构和磁性能进行了表征。结果表明：通过化学镀工艺制备的Ni-P合金镀层厚度约为4 μm，且为非晶结构，并具有一定的磁性；该磁性ICF靶丸可望用来进行磁悬浮实验研究。最后，对聚苯乙烯靶丸表面磁性涂层的制备机理进行了讨论。     

磁性流体薄片高电压电流光学测量的研究

研究一种用磁性流体薄片对高压电流进行光学测量的电流传感器。设计原理基于磁性流体的光透射率随垂直磁场强度的变化而变化的关系。磁性流体受到垂直外磁场作用,原先无序的磁性颗粒将凝聚在一起形成条条磁链,从而引起磁性流体的光透射率的变化。采用磁性流体作为传感媒介设计的传感结构避免了基于法拉第效应的光磁式电流互感器对环境干扰敏感造成信噪比不高和传统的电磁式电流互感器的高压绝缘的缺陷。通过改变磁性流体的浓度和基液,或者改变传感头的结构,来达到实际需要的传感灵敏度和响应时间。     

水平圆管内磁性潜热型功能流体对流换热特性的数值模拟

建立磁场作用下水平圆管内磁性潜热型功能流体对流换热的数学物理模型,分析磁场强度、磁性相变微胶囊体积分数、流体质量流量等因素对流体对流换热的影响.磁场对磁性潜热型功能流体的对流换热具有显著的强化作用,磁场强度愈大强化作用愈明显,强化原因是磁性相变微胶囊受到磁力作用产生扰动.     

磁性流体及其应用

磁性流体是一种强磁性液体,是用 100以下的F3O4等磁性微粒稳定地分散在水和油中形成的磁性胶体溶液,在重力和磁场的作用下也不发生凝聚和沉淀. 1965年美国的Papell首先研制成功磁性流体.在七十年代后期,美、日、苏和英等国的研究工作迅速发展,美国还成立了专门生产磁性流体和开     

磁性荧光粉的制备方法及其性能和应用的研究

本文叙述了磁性荧光粉的制备方法、性能和使用方法;探讨了在制备过程中影响荧光亮度和磁力强度的一些主要因素;并研究了磁性荧光粉在水介质中使用时的分散情况.确定了制取优质磁性荧光粉的最佳条件,以及配制水磁悬液时所采用的分散剂的种类和条件.同时与日、美同类产品在技术性能上做了比较.     

Heat capacities of the dipolar Yukawa model polar fluid

The Stockmayer fluid is often used to describe a polar fluid. The dipolar Yukawa (DY) fluid is also a useful model for such fluids and is convenient for theoretical applications. Here we use the mean spherical approximation (MSA) and perturbation theory (PT) to study the heat capacities of the DY fluid model of a polar fluid and compare these results with Monte Carlo simulations for this model polar fluid. We find that the DY fluid shows the same features as the Stockmayer fluid does; demonstrating the utility of the DY fluid and further finding that the MSA and PT approaches give reasonably accurate results for the heat capacity.     

五维地震油气识别方法*

五维地震流体识别,即利用五维地震资料对复杂储层含流体特征进行识别和描述,为业内研究的前沿和重要难题。该文首先从岩石物理机制出发,研究了含流体各向异性储层参数与物性参数的关系,构建了高敏感参数的各向异性因子f^ani,并验证了该流体因子的合理性以及实用性。其次,利用各向异性反演算法尽可能地挖掘五维地震数据中丰富的方位各向异性信息,反演得到用来表征地下流体的各向异性因子,实了现五维地震流体识别。实际应用结果表明,基于新的各向异性因子及各向异性反演算法能够稳定可靠地从五维地震数据中获取储层流体特征,为五维地震流体识别提供了一套新的理论方法。     

Streamer radius model and its assessment using two-dimensionalmodels

The variable radius method is proposed to approximate the radius of the ionization channel in the one and a half-dimensional (1.5-D) fluid models for studying streamer development, in which the unreasonable constant radius in the traditional 1.5-D fluid models is corrected. The streamer development and propagation between the 1.5-D fluid model with the variable radius method and the two-dimensional (2-D) fluid model using the same initial and external conditions are compared. The radius in each stage of streamer development from the 1.5-D fluid model with the variable radius method shows agreement to a certain degree with that of the 2-D fluid model. The purpose of this paper is not to negate the role of the 2-D fluid models, but to explore the potential of the 1.5-D fluid models and make them more useful and accurate as well as to understand the evolution of streamer radius. The streamer development from the 1.5-D fluid model with the variable radius method not only maintains simplicity of the 1.5-D fluid models, but also presents agreement with the 2-D fluid models for streamers     

Exact Solutions for the Flow of Fractional Maxwell Fluid in Pipe-Like Domains

This paper presents an analysis of unsteady flow of incompressible fractional Maxwell fluid filled in the annular region between two infinite coaxial circular cylinders. The fluid motion is created by the inner cylinder that applies a longitudinal time-dependent shear stress and the outer cylinder that is moving at a constant velocity. The velocity field and shear stress are determined using the Laplace and finite Hankel transforms. Obtained solutions are presented in terms of the generalized G and R functions. We also obtain the solutions for ordinary Maxwell fluid and Newtonian fluid as special cases of generalized solutions. The influence of different parameters on the velocity field and shear stress is also presented using graphical illustration. Finally, a comparison is drawn between motions of fractional Maxwell fluid, ordinary Maxwell fluid and Newtonian fluid.     

基于Poiseuille流动的汽车磁流变减振器分析与测试

利用牛顿流体模型和滨汉流体模型,对基于Poiseuile流动的汽车磁流变减振器进行了分析,设计制作了微型汽车磁流变减振器,并对此进行了测试,测试结果表明：所提出的分析方法是可行的,对设计汽车磁流变减振器有一定的指导意义。     

微通道疏水表面滑移的耗散粒子动力学研究

了解疏水表面的滑移规律对其在流动减阻方面的应用至关重要.利用耗散粒子动力学(dissipative particle dynamics, DPD)方法研究了微通道疏水表面的滑移现象.采用固定住的粒子并配合修正的向前反弹机制,构建了DPD固体壁面边界模型,利用该边界模型模拟了平板间的Couette流动.研究结果表明,通过调整壁面与流体间排斥作用强度,壁面能实现从无滑移到滑移的转变,壁面与流体间排斥作用越强,即疏水性越强,壁面滑移越明显,并且滑移长度与接触角之间存在近似的二次函数关系.无滑移时壁面附近密度分布均匀,有滑移时壁面附近存在低密度区域,低密度区域阻碍了动量传递,致使壁面产生滑移.     

Plane waves in noncommutative fluids

We study the dynamics of the noncommutative fluid in the Snyder space perturbatively at the first order in powers of the noncommutative parameter. The linearized noncommutative fluid dynamics is described by a system of coupled linear partial differential equations in which the variables are the fluid density and the fluid potentials. We show that these equations admit a set of solutions that are monochromatic plane waves for the fluid density and two of the potentials and a linear function for the third potential. The energy–momentum tensor of the plane waves is calculated.     

Density Functional Approach Based on Numerically Obtained Bridge Functional

The Ornstein Zernike equation is solved with the Rogers Young approximation for bulk hard sphere fluidand Lennard-Jones fluid for several state points. Then the resulted bulk fluid radial distribution function combinedwith the test particle method is employed to determine numerically the function relationship of bridge functional as afunction of indirect correlation function. It is found that all of the calculated points from different phase space statepoints for a same type of fluid collapse onto a same smooth curve. Then the numerically obtained curve is used tosubstitute the analytic expression of the bridge functional as a function of indirect correlation function required in themethodology [J. Chem. Phys. 112 (2000) 8079] to deterrnine the density distribution of non-uniform hard spherefluid and Lennard Jones fluid. The good agreement of theoretical predictions with the computer simulation data isobtained. The present numerical procedure incorporates the knowledge of bulk fluid radial distribution function intothe constructing of the density functional approximation and makes the original methodology more accurate and moreflexible for various interaction potential fluid.     

Accretion onto a born-Infeld black hole

This study deals with the accretion of an isotropic fluid onto a Born-Infeld black hole. For this purpose, we have formulated the fluid velocity $u\left(r\right),$ energy density $\varrho \left(r\right)$ and rate of mass accretion for a singularity free black hole with the help of the barotropic equation of state and conservation laws. We have plotted the governing results to inspect the physical significance of the matter flow around the specific black hole. The spherically symmetric accretion has been analyzed for a stiff fluid, dust fluid, quintessence fluid and phantom fluid. The plotted critical quantities have been discussed by finding the critical radius, and all the plots have been shown in two regions. The fluid velocity and the energy density have positive and negative regions. It has been found that the black hole mass increases for the stiff fluid, dust fluid and quintessence fluid, but it decreases for the phantom fluid.     

浮升力和流动加速对超临界CO2管内流动传热影响

基于单相流体的概念,超临界流体的异常传热行为已经被研究很多年了,但是关于其流动传热机理仍没有统一的认识.本文通过理论分析和实验研究了超临界二氧化碳在竖直管内向上流动过程中,浮升力和流动加速效应对其流动结构和传热过程的影响.结果表明,没有确凿的实验证据表明超临界流体的异常传热行为是浮升力和流动加速直接导致的,存在的估计浮升力和流动加速效应准则均是在常物性流体的基础上,做了大量假设得出的,不同的研究者采用浮升力和流动加速准则分析超临界流体的传热恶化得出的结论不一致.最后,基于拟沸腾理论分析超临界流体的传热恶化过程,提出超临界沸腾数区分了超临界流体正常传热与恶化传热的转换边界,为超临界流体流动传热研究提供新思路,超临界沸腾数对建立用于不同技术的超临界流体动力循环的最佳运行条件具有重要意义.