Propagation of cylindrical and spherical dust–ion acoustic solitary waves in a relativistic dusty plasma

The properties of cylindrical and spherical dust–ion acoustic solitary waves (DIASW) in an unmagnetized dusty plasma comprising of relativistic ions, Boltzmann electrons, and stationary dusty particles are investigated. Under a suitable coordinate transformation, the cylindrical KdV equation can be solved analytically. The change of the DIASW structure due to the effect of geometry, relativistic streaming factor, ion density and electron temperature is studied by numerical calculation of the cylindrical/spherical Kdv equation. It is noted that with ion pressure the effect of relativistic streaming factor to solitary waves structure is different. Without ion pressure, as the relativistic streaming factor decreases, the amplitude of the solitary wave decreases. However, when the ion pressure is taken into account, the amplitude decreases as the relativistic streaming factor increases and is highly sensitive to relativistic streaming factor. Our results may have relevance in the understanding of astrophysical plasmas.     

表面张力贮箱泡破点盲测技术研究

通过对表面张力贮箱结构、泡破点测试难点分析,提出了采用微压闭环控制技术解决测试过程管理装置内腔压力维持准平衡状态难题的技术途径,研制的贮箱泡破点盲测系统具有自动控制、自动判读及测试精度高等特点,经试验验证该技术满足贮箱泡破点盲测要求,已在型号研制中得到应用。     

VASIMR中螺旋波等离子体源设计

螺旋波等离子体具有密度高,可控性强且无电极等优点,被应用于可变比冲磁等离子体火箭(VASIMR,Variable Specific Impulse Magnetoplasma Rocket)中.设计了一个螺旋波等离子体源,并给出了其中2个关键部分——磁场线圈和螺旋波天线的设计.对螺旋波等离子体源进行了初步实验,结果表明,电子密度随射频输入功率的增加几乎呈线性上升,估计电子密度的量级在通入工质后完全可达10¹¹ cm^-3.     

Nonlinear electromagnetic perturbations in a degenerate electron–positron plasma

Nonlinear propagation of fast and slow magnetosonic perturbation modes in an ultra-cold, degenerate (extremely dense) electron–positron (EP) plasma (containing non-relativistic, ultra-cold, degenerate electron and positron fluids) has been investigated by the reductive perturbation method. It is shown that due to the property of being equal mass of the plasma species (_me=_mp$m_e=m_p$, where _me$m_e$ and _mp$m_p$ are electron and positron mass, respectively), the degenerate EP plasma system supports the K-dV solitons which are associated with either fast or slow magnetosonic perturbation modes. It is also found that the basic features of the electromagnetic solitary structures, which are found to exist in such a degenerate EP plasma, are significantly modified by the effects of degenerate electron and positron pressures. The applications of the results in an EP plasma medium, which occurs in compact astrophysical objects, particularly in white dwarfs, have been briefly discussed.     

Vertical TEC variations and model during low solar activity at a low latitude station,Xiamen

GPS-derived vertical TEC recorded at Xiamen (24.5°N, 118.1°E, geomagnetic latitude 13.2°N), China, during year 2006 is analyzed for the first time and compared to that predicted by ionosphere model SPIM recommend by ISO. A manifest seasonal anomaly is found with the high value during equinoctial season and low value during summer and winter season. Relative standard deviation for VTEC shows high value at around midnight and before sunrise. The correlation analysis exhibits that the variation of VTEC has a very weak relation with geomagnetic and solar activities (Dst, AP, SSN and F10.7). Comparative results reveal that the SPIM overestimates the observed VTEC at most of the time.     

基于遗传算法的柴油机喷油系统模型参数辨识

柴油机喷油系统中压力的变化会引起气泡的产生和溃灭,而气泡的变化会对燃油的流动和压力波的传播产生影响.为了更准确预测喷油系统中的初始含气率以及变化情况,提出了应用改进遗传算法对柴油机喷油系统模型中的柱塞腔、出油阀紧帽腔、高压油管和针阀腔初始含气率进行辨识的新方法.基于气泡模型,建立了气-液两相条件下的柴油机喷油系统模型,通过仿真数据和试验数据对比,构造了适应度函数,实现了对柴油机喷油系统模型的参数辨识,并得到了参数优化后的柴油机喷油系统模型.仿真结果与试验数据的比较验证了采用改进遗传算法对气-液两相条件下的柴油机喷油系统模型进行参数辨识的可行性.     

低雷诺数下层流分离的等离子体控制

为有效控制层流分离特性,消除或减弱低雷诺数时小迎角下的升力非线性现象,改善翼型升力特性,并通过翼型的上表面转捩带与油流显示测量对等离子体激励控制机理进行阐述,对厚度为16%椭圆翼型低雷诺数下的气动特性进行了风洞试验研究。在此基础上,在上表面前缘10%弦长处布置激励器,通过压力分布测量观察等离子体激励对层流分离的影响。试验结果表明：当翼型上表面仅发生层流分离时,等离子体激励和转捩带的作用类似,可以有效延迟或者消除后缘层流分离,从而增加升力;当翼型上表面出现层流分离气泡并发生再附现象时,等离子体可以有效减小或者消除层流分离泡的范围,从而减小升力;通过控制层流分离,占空循环等离子体激励可以实现对低雷诺数小迎角下的升力的线性控制。     

转捩对压缩拐角激波/边界层干扰分离泡的影响

为了研究转捩对压缩拐角内分离泡结构的影响,进行了来流马赫数2.9,24°压缩拐角激波/转捩边界层干扰的直接数值模拟（DNS）。通过在拐角上游平板的不同流向位置处添加周期性吹吸扰动激发流动转捩,使得转捩不同阶段进入拐角入口,从而在拐角内产生激波/转捩边界层的相互干扰。计算得到的平均速度剖面、壁面压力分布以及分离泡大小与风洞试验及以往直接数值模拟结果吻合较好,验证了计算结果的可靠性。研究了转捩过程对角部干扰区内分离泡结构的影响规律,分析比较了不同转捩阶段下角部分离区内湍动能的生成、耗散和分配机制。研究结果表明：转捩初期的拟序涡结构对分离泡尺度及形状影响最大,发卡涡包在角部拐点附近发生展向融合,并在角部区域形成湍流斑,此时分离泡尺度最小,形状呈现中间高两边低的山峰型。随着转捩的发展,分离区内湍动能生成和近壁区的耗散逐步降低,此时输运项起到了主要的平衡作用。     

IRI-2007预测TEC在广州地区的适用性分析

利用广州站(23.2°N, 113.3°E) GPS双频接收机监测的电离层TEC数据和IRI-2007模型不同电离层输入参数计算得到的TEC预测值, 对比分析了太阳活动低年(2008年)广州地区TEC的变化特征. 结果表明, TEC观测值周日变化在16:00LT左右达到最大值, 而IRI-TEC最大值出现时间较GPS-TEC提前1h左右. TEC季节变化在春秋分较高, 两至季节较低, 表现出明显的半年特性和季节依赖性, 并出现冬季异常现象. IRI-TEC与GPS-TEC在白天具有较好的一致性, 夜间偏差较大. 不同电离层输入参数得到的TEC预测值也相差较大, 选用顶部电子密度参数NeQuick、底部厚度参数B0 Table并用URSI系数计算F₂层峰值参数时, 能较好地反映TEC观测值的变化特征. 在对磁暴的响应上, 预测值无明显变化, 观测值则有比较明显的表现. 通过对比, 初步分析了利用IRI-2007模型预测TEC在广州地区的适用性, 并给出了合理的参数选择方案.      

Dust Acoustic Wave in Dusty Plasmas With Streaming Ions Under Ultraviolet Irradiation

The reductive perturbation method is applied to investigate the dust acoustic soliton in dusty plasmas with streaming ions under ultraviolet irradiation theoretically and numerically. The self-consistent dust charge variation is taken into account. It is shown that the ultraviolet irradiation can significantly lower the magnitude of the dust negative charge, and ion streaming velocity firstly raise the magnitude of the dust negative charge and then lower it. With the growth of (Ultraviolet) UV photo flux or ion streaming velocity, the phase velocity and width of the solitary waves decrease, whereas its amplitude increases.