医药洁净室的计算流体动力学模拟及实测对比

采用计算流体动力学(CFD)模拟,研究3个医药洁净室的气流流型及颗粒物浓度.采用标准k-ε双方程模型,通过模拟颗粒物在洁净室的分布,分析合理的污染物散发位置及散发比例.对比参考发尘量下的结果与实测数据的差异,根据实测数据确定污染散发量,通过试验不同的单位容积发尘量,计算对应的洁净度,得到与实测数据吻合最好的单位容积发尘量.在单位容积发尘量为1 000pc·(m3·min)-1计算条件下,各房间的模拟结果与实测数据数值比较吻合,且经CFD预测的3个房间的洁净度变化趋势与实测一致.     

高静态动作压力下粉尘爆炸泄放标准的可靠性

粉尘爆炸泄放设计标准的可靠性对能否实现爆炸防护尤为关键.以中径70μm石松子粉尘为介质,采用20 L球形粉尘爆炸装置进行了4种泄放口径、静态动作压力在0.12~0.6 MPa的爆炸泄放实验,对比了实验值与NFPA 68和EN 14491计算值.结果表明,NFPA 68在预测高静态动作压力下的泄放面积时,随着泄放口径的增大,预测结果由保守变为危险,但预测结果精度较好且数值稳定;EN 14491在预测高静态动作压力下的泄放面积时非常保守,预测精度较差,数据不可靠.依据两种标准推荐的经验函数关系,分析了NFPA 68和EN 14491在预测高静态动作压力时产生这种差异的原因.     

Analytical Study of Nonlinear Dust Acoustic Waves in Two-Dimensional Dust Plasma with Dust Charge Variation

The nonlinear dust acoustic waves in two-dimensional dust plasma with dust charge variation is analytically investigated by using the formally variable separation approach. New analytical solutions for the governing equation of this system have been obtained for dust acoustic waves in a dust plasma for the first time. We derive exact analytical expressions for the general case of the nonlinear dust acoustic waves in two-dimensional dust plasma with dust charge variation.     

尘埃粒子的时空结构及其性质

讨论了尘埃粒子解的时空结构及其性质，导出了尘埃粒子的内空间的离散结构.证明了尘埃粒子内部的物质球是一个无坐标的平直球，因而具有最小的体积和整体的关联性.导出了在尘埃粒子的内外时空中的径向测地线并说明其连续性.阐述了由这个解所揭示的物质、引力与时空之间的内在联系. 关键词： 尘埃粒子 离散时空 测地线     

The Study of MMW and MW Attenuation Considering Multiple Scattering Effect in Sand and Dust Storms at Slant Paths

The influence of sand and dust storms on modern MMW and satellite communication systems reliability have been paid more attention to. The attenuations induced by sand and dust storms are estimated by means of Mie-theory and Rayleigh approximation, in the case of the tenuous distribution of particles. With the particle density increasing, however, these method become inadequate, the multiple scattering effects then become dominant for attenuation estimation. The attenuations considering multiple scattering effects are estimated by Monte-Carlo and four fluxes method at horizontal paths. At slant paths, based on multi-layer media model, the attenuations considering multiple scattering effects are calculated by layered Monte-Carlo method at 100, 37, 24, and 14GHz. It is shown that the multiple scattering effects should be considered at the attenuation prediction in the sand and dust storm, which the visibility is about 0.5km and smaller than 0.5km and frequency is about 20GHz. Above 30GHz, the multiple scattering effects due to sand and dust particles should be considered, as visibility is about 1km and smaller than 1km at slant paths.     

Letter: Causality Violating Geodesics in Bonnor's Rotating Dust Metric

We exhibit timelike geodesic paths for a metric, introduced by Bonnor [11] and considered also by Steadman [13], and show that coordinate time runs backward along a portion of these geodesics.     

实现细粒煤深度脱硫产业化的研究

根据我国高硫煤的赋存特点,提出采用微细介质重介旋流器及细泥选择性絮凝组合工艺实现细粒煤的深度脱硫,无机硫脱除率可大幅度提高,分选下限明显降低,是实现煤炭深度脱硫降灰产业化的有效技术途径.     

收尘极板上沉降粉尘粘结性能研究

振打清灰效果不好，严重影响电除尘器的除尘效率和使用范围，而影响振打清灰效果的最主要因素是沉降粉体的粘结力。通过建立数学模型从微观的角度推导出粉尘之间各种粘结力的理论计算公式。分析了比电阻、外加电场和粉尘含水率等因素对粉尘粘结力的影响。在实验中，模拟电除尘器中的静电场，测出在不同外加电场下粉尘粘结力的大小，定量的反应了外加电场对粉尘粘结性能的影响。     

炼钢厂引风机叶轮粘灰控制

对目前广泛采用的炼钢厂一次烟气引风机叶轮冲水清灰效果不佳的原因进行了分析，提出采用压缩气体清灰的思路，并计算了供气压力。现场实际运行效果表明，风机运行周期超过1个月。     

Charge density fluctuation of low frequency in a dusty plasma

The charge density fluctuation of low frequency in a dusty plasma, which is derived from the longitudinal dielectric permittivity of the dusty plasma, has been studied by kinetic theory. The results show that theP value, which describes the relative charge density on the dust in the plasma, and the charging frequency of a dust particle Ω _c , which describes the ratio of charge changing of the dust particles, determine the character of the charge density fluctuation of low frequency. For a dusty plasma ofP≪1, when the charging frequency Ω _c , is much smaller than the dusty plasma frequency ω_d, there is a strong charge density fluctuation which is of character of dust acoustic eigenwave. For a dusty plasma ofP≫1, when the frequency Ω _c , is much larger than ω _d there are weaker fluctuations with a wide spectrum. The results have been applied to the ionosphere and the range of radius and density of dust particles is found, where a strong charge density fluctuation of low frequency should exist.