某型滑轨组件焊接工艺研究

某型滑轨组件采用结构钢基体与厚度为1.5mm的无油自润滑轴承衬板焊接而成。结构钢基体采用18Cr2Ni4WA材料,具有支撑、保证整体刚性的作用。将自润滑衬板冲压成形与滑轨紧密贴合后,边缘采用电子束焊接工艺进行连接。提出一种抗脱落、耐摩擦、精度高、摩擦系数小、成本低、能承受较大载荷的高压燃油柱塞泵滑轨的结构设计方案及加工工艺。     

激光能量沉积降低钝头体驻点压力机制分析

针对高超声速飞行器表面驻点压力较高的问题,在马赫数5的来流条件下,分别采用单脉冲和高重频激光能量注入的方式控制弓形激波。将数值模拟结果与高时空分辨率纹影照片以及驻点压力测量结果相对比,分析了单脉冲激光能量与高超声速流场弓形激波的相互作用过程,结果表明透镜效应是激光能量沉积降低钝头体驻点压力的原因。单脉冲激光能量产生的低压区不能维持,降低驻点压力效率低,因此高重频是更有效的激光能量注入方式。优化了频率为80kHz、功率为自由流焓流6.6%的激光能量沉积位置,计算结果表明当沉积位置与钝头体表面的距离等于钝头体直径的1.5倍时,驻点压力降低了40%。在优化位置提高沉积能量大小至36.9%,可将驻点压力和热流分别降低83.3%和56.9%。     

水汽对折光修正精度的影响分析

针对当前部分折光修正的工程应用常常忽略水汽影响的现状,选取了国内4个不同地域的气象站点,基于1995年的数百组历史气象探空数据,利用射线描迹法分别仿真计算包含水汽和忽略水汽2种情况下由于大气折射引起的测距误差和测角误差,并对这4个站点不同仰角和不同时间的测距偏差和测角偏差进行统计分析,结果表明：水汽是构成测量残差的一个重要误差源,对于精度要求较高的折光修正系统,水汽的影响不能忽略.该分析结果可为其他需要考虑大气折射效应影响的高精度光学测量工程领域提供参考.     

固冲发动机补燃室非稳态沉积过程分析

采用随机轨道模型,基于动网格技术,分析了固冲发动机补燃室非稳态沉积过程中燃气流动边界形状变化对燃气流动及沉积分布的影响,得到了补燃室内壁面的非稳态沉积规律,对直连试验中出现的进气道出口拐角烧蚀沟槽现象进行了理论分析。研究发现,不同粒径的粒子在补燃室内的分布特性差异较大;凸起的沉积块可改变燃气流向,使进气道出口拐角处的高温区变大,易形成沟槽;点火初期,掺混区进气道之间的沉积速率较大。     

跑道拼接工程对道面的影响

以虹桥国际机场飞行区扩建工程为依托,通过对拼接区域进行跑道表面沉降及周边土体竖向位移、水平位移、孔隙水压力和地下水位等项目的监测．对新建联络道与既有跑道的拼接工程不停航施工对跑道道面性能的影响进行全面监测与分析。监测结果表明,拼接工程引起的道面沉降量较小,超过60％的测点竖向位移小于3mm;拼接工程对周边土体地下水位没有影响：拼接工程会引起周边土体产生超孔隙水压力。最大可达到正常孔隙水压力的2倍,工后1年基本消散;拼接工程会引起周边土体产生竖向和水平向位移．影响程度随深度增加而减少,影响深度不超过7m。研究表明,通过采取合适的施工方案及必要的防范措施．拼接段施工不会影响跑道的正常使用。     

航空发动机燃烧室喷嘴内部燃油结焦研究

对在最严重热负荷时喷嘴内部燃油沉积率以及燃油性能参数的变化进行了试验研究。对1个相似的喷嘴试验件进行了传热试验,通过试验修正计算中关键的传热系数,建立了符合喷嘴实际的传热计算方法;用该方法推算发动机在真实条件下发生最严重热负荷的工况,然后进行了燃油沉积率试验,得到了燃油管道沉积率与温度的关系,同时得到了喷嘴和油滤上积沉的特征;对沉积物成分进行了分析,并测定了燃油油样进行性能参数。通过研究结果,提出了改善喷嘴燃油热安定性的措施。     

Electron density retrieval from occulting GNSS signals using a gradient-aided inversion technique

In the coming years, opportunities for remote sensing of electron density in the Earth’s ionosphere will expand with the advent of Galileo, which will become part of the global navigation satellite system (GNSS). Methods for accurate electron density retrieval from radio occultation data continue to improve. We describe a new method of electron density retrieval using total electron content measurements obtained in low Earth orbit. This method can be applied to data from dual-frequency receivers tracking the GPS or Galileo transmitters. This simulation study demonstrates that the method significantly improves retrieval accuracy compared to the standard Abel inversion approach that assumes a spherically symmetric ionosphere. Our method incorporates horizontal gradient information available from global maps of Total Electron Content (TEC), which are available from the International GNSS Service (IGS) on a routine basis. The combination of ground and space measurements allows us to improve the accuracy of electron density profiles near the occultation tangent point in the E and F regions of the ionosphere.     

Peculiarities of the nighttime winter foF2 increase over Irkutsk

An analysis of properties and peculiarities of the nighttime winter foF2 increases (NWI) in the East Siberia is made on data of ionospheric station Irkutsk in the periods 1958–1992 and 2002–2009 and the empirical model of the F2 layer critical frequency under the geomagnetic quiet conditions deduced from these data (model Q-F2). It is revealed, that the NWI is the stable regularity of the quiet ionosphere over Irkutsk. The amplitude of the NWI (the difference between maximum and minimum foF2 values at night hours) is the greatest in December–January and nearly the same at low and middle solar activity. It is a peculiarity of the quiet ionosphere in the East Siberia. Maximum in night foF2 under quiet geomagnetic conditions is observed mainly after midnight (02-04 LT) and is shifted to predawn hours as solar activity increases. At low solar activity the quiet ionosphere at ∼02–04 LT shows the following properties: (a) the fluctuations of foF2 and hmF2 are in the reverse correlation but this dependence is weak; (b) very strong fluctuations of foF2 (|δfoF2| > 30%) occur seldom (∼4% of events) and almost all of them are positive; an example of very strong fluctuations of foF2 up to 60% can be an extreme increase in the foF2 on 19.12.2008; (c) the very strong enhancements of foF2 in the NWI maximum can be observed at the low geomagnetic activity, they occur more often during substorms but very seldom during geomagnetic storms. Possible reasons of these properties of NWI are discussed.     

Possible interstellar anions: CnS and CnO (n = 2–8)

The geometries, electron affinities and/or electron detachment energies for the C_nS and C_nO (n = 2–8) molecules and their anions were calculated by using the RCCSD (T) method. The C_nS⁻ (even n = 4, 6, and 8) and C_nO⁻ (even n = 6 and 8) anions are found to be substantially more stable than their corresponding neutral species. Several anions are potentially detectable as interstellar molecules.     

Coupling plasma plume of a low-power magnetically shielded Hall thruster with a hollow cathode

The coupling region of a Hall thruster with a hollow cathode is the region between the cathode and the thruster plume. The characteristics of plasma in that region are complicated and strongly associated with the thruster working conditions and the cathode position. In this paper, a laboratory 100 W class magnetically shielded Hall thruster was coupled with a hollow cathode. Optical imaging and electrostatic probe were employed to monitor and scan the plasma plume. Plume characteristics in the coupling region in non-self-sustained mode and self-sustained mode were compared. Evolution of the coupling plume with the cathode position was studied. Experiments show that, when turning the thruster into self-sustained mode or moving the cathode further away axially, the discharge current can be reduced by 6.4–10.6% restraining the electron current and improving ionization. In particular, when the cathode is moved further, the electron conduction near the channel walls is suppressed. The electron current is reduced by 27.4% and the ion beam current is increased by 7%. Overall, this work shows that the working mode of the thruster and the position of the cathode greatly affect the coupling plasma plume. Both play an important role in improving the utilizations of propellant and current.