加力燃烧室用气冷喷油杆结焦特性数值研究

为阐明实际工作环境参数下气冷喷油杆内燃油结焦速率与沉积厚度等特性,建立沿喷杆轴向的一维非稳态热-流-固耦合换热与燃油结焦计算模型,获得了喷杆壁面与燃油温度、结焦速率与相对结焦厚度等参数沿程分布。分析了燃油进口温度和质量流量对燃油结焦特性的影响,并与无气冷喷杆方案结果进行了对比。计算结果表明:燃油温度沿轴向逐渐升高,喷杆壁温在底端达到峰值。基准工况下气冷喷杆结焦速率和结焦厚度均沿轴向先升高后降低。结焦速率最大为26μg/(cm2·h),对应相对结焦沉积厚度0.6%。无气冷喷杆方案,在喷杆前端和底部各存在一结焦峰值区域。结焦速率峰值分别为398μg/(cm2·h)和807μg/(cm2·h),对应相对结焦沉积厚度8%和15%。固定燃油进口流量,随着燃油进口温度升高,结焦速率显著增大,喷杆内结焦总质量呈指数级增长趋势。固定燃油进口温度,进口流量越大,结焦速率略有增大,结焦总质量仅呈线性增长趋势。相较于无气冷喷杆,气冷喷杆可显著降低喷杆壁面与燃油温度,从而大幅抑制结焦生成。     

直流滑动弧等离子体点火器特性的实验研究

为了探究直流滑动弧放电应用于航空发动机燃烧室内点火的性能特点,设计了直流滑动弧等离子体点火器,在模型燃烧室内进行了煤油/空气混合气的点火实验,利用高速相机记录了滑动弧等离子体点火器的电弧产生和滑动过程以及燃烧室内煤油/空气混合气的点火和火焰发展过程,研究了不同空气工作介质流量、驱动电源输出电流、点火器电极夹角和点火器安装位置等因素对滑动弧等离子体点火器点火特性的影响。结果表明:滑动弧在运动过程中会产生不规则的跳动,并且存在着电弧分流的现象,导致电弧长度发生变化;在湍流的作用下,初始火核会演变为分裂的、大面积的湍流火焰,着火面积不断增大,最终在t=21ms时形成稳定燃烧;随着空气工作介质流量增大、驱动电源输出电流减小以及点火器的安装位置远离燃油雾化喷嘴,滑动弧等离子体点火器的电弧长度减小,点火延迟时间逐渐增长,例如余气系数α=8时,I=30A下电弧长度为47.1mm,相比I=20A增长了75.1%,点火延迟时间为21ms,相比I=20A缩短了40%;而随着点火器电极夹角的增大,电弧长度先增大后减小,点火延迟时间则先减小后增长,在电极夹角θ=45°时,电弧长度最长,点火延迟时间最短,分别为30.5mm和12ms。     

不同几何结构对燃油喷嘴热防护特性的影响

试验研究了不同管路结构对燃油结焦性能的影响,结果表明,在1 000 K、150 m/s来流条件和400 K、05 m/s燃油条件下,减小弯管角度和突扩管路的突扩尺寸可以降低结焦附着,且在对管路加热的初始阶段中,结焦量随时间增加会出现波动,在加热15 min时管壁结焦量达到最大,壁面上部分结焦的脱落使结焦量降低。随后,采用试验与数值模拟相结合的方法研究了喷嘴和喷嘴帽罩结构对热防护特性的影响。结果表明,主、副油路同心布置的喷嘴具有最好的热防护效果,在所试验工况下最高可降低湿壁温度近50%,甚至优于带空气隔热层的模型。而喷嘴帽罩对喷嘴出口油温的降低有限,但减小帽罩与喷嘴体的接触或在接触面处填充低热导率的材料仍是有效的改进措施,可降低出口油温约5 K。研究结果对喷嘴的热防护设计具有指导作用。     

Microstructure and mechanical properties of hybrid fabricated 1Cr12Ni2WMoVNb steel by laser melting deposition

 Laser melting deposition was carried out to deposit a 1Cr12Ni2WMoVNb steel bar on a wrought bar of same material. Room-temperature tensile properties of the hybrid fabricated 1Cr12Ni2WMoVNb steel sample were evaluated, and microstructure, fracture surface morphology, and hardness profile were analyzed by an optical microscope (OM), a scanning electron microscope (SEM), and a hardness tester. Results show that the hybrid fabricated 1Cr12Ni2WMoVNb steel sample consists of laser deposited zone, wrought substrate zone, and heat affected zone (HAZ) of the wrought substrate. The laser deposited zone has coarse columnar prior austenite grains and fine well-aligned dendritic structure, while the HAZ of the wrought substrate has equiaxed prior austenite grains which are notably finer than those in the wrought substrate zone. Besides, austenitic transformation mechanism of the HAZ of the wrought substrate is different from that of the laser deposited zone during the reheating period of the laser deposition, which determines the different prior austenite grain morphologies of the two zones. Microhardness values of both the laser deposited zone and the HAZ of the wrought substrate are higher than that of the wrought substrate zone. Tensile properties of the hybrid fabricated 1Cr12Ni2WMoVNb steel sample are comparable to those of the wrought bar, and fracture occurs in the wrought substrate zone during the tensile test.     

消融控制电弧等离子体发生器放电特性的实验研究

通过衬套材料消融补充等离子体从而控制电弧生长的技术具有很好的应用前景。利用一个总贮能800kJ的模块化电容基脉冲功率源系统为消融控制电弧等离子体发生器强流放电提供电能输入，在一定的参数变化范围内，实验研究了脉冲功率源初始放电参数、等离子体发生器几何参数以及消融材料对消融控制电弧放电特性的影响规律。借助于理论分析，也可定性获得消融控制电弧等离子体压力和温度对上述影响参量变化的依赖关系。     

Thermospheric neutral density response to solar forcing

Recent measurements by the Solar EUV (Extreme Ultra Violet) Experiment (SEE) aboard the Thermosphere–Ionosphere–Mesosphere Energetics and Dynamics satellite (TIMED) provide solar EUV spectral irradiance with adequate spectral and temporal resolution, and thus the opportunity to use solar measurements directly in upper atmospheric general circulation models. Thermospheric neutral density is simulated with the NCAR Thermosphere–Ionosphere–Electrodynamic General Circulation Model (TIEGCM) using TIMED/SEE measurements and using the EUVAC solar proxy model. Neutral density is also calculated using the NRLMSISE-00 empirical model. These modeled densities are then compared to density measurements derived from satellite drag data. It is found that using measured solar irradiance in the general circulation model can improve density calculations compared to using the solar proxy model. It is also found that the general circulation model can improve upon the empirical model in simulating geomagnetic storm effects and the solar cycle variation of neutral density.     

电弧增材制造7075铝合金的微观组织与力学性能

7xxx系铝合金电弧增材制造过程中因组织不均匀与元素偏析导致成形试样性能较低,针对这一问题,对电弧增材制造7075铝合金薄壁件进行固溶+人工时效热处理(T6态),对比研究了热处理前后微观组织与力学性能的变化。结果表明,7075铝合金沉积态试样中晶粒被网状共晶组织包围,Zn、Mg和Cu元素在晶界富集,产生元素偏析。经过T6态热处理后,大部分共晶组织溶解,元素分布的不均匀性得到明显改善。与沉积态试样相比,热处理后试样的抗拉强度与断后伸长率增加,抗拉强度从(279.4±5.3)MPa提高至(493.9±10.2)MPa,断后伸长率从3.78%±0.35%增加到9.66%±1.70%。T6态试样的拉伸断口表面密布着韧窝,断裂方式为韧性断裂。     

Preliminary evidence for drizzle in the middle cloud layer of Venus

Vertical trajectory data from the VEGA 1 and 2 balloon flights in the atmosphere of Venus is re-analyzed. A previously employed helium leak rate profile invoked to entirely account for the decrease in equilibrium float altitude of VEGA 2 is questioned and deemed ad hoc. As an alternative, it is proposed that both VEGA 1 and 2 experienced in-flight mass increases due to the deposition of cloud particles onto their envelopes, as well as losing helium at a reduced rate consistent with the pre-flight prediction. Particle deposition rates are estimated and found to be compatible with this alternative scenario. Possible evidence for drizzle is also presented. Preliminary experiments to derive aerosol deposition rate on a flat plate and the maximum feasible liquid mass that may be accumulated on a near-spherical envelope are briefly described. Further experimental work is recommended to constrain the deposition efficiency values involved and the maximum feasible drizzle fluxes that could have been encountered by both VEGA 1 and 2.     

A genetic algorithm for Initial Orbit Determination from a too short arc optical observation

Optical observations constitute a source of angular measurements of a satellite pass. Commonly, these observations have short durations with respect to the satellite orbit period. As a consequence, the use of classical orbit determination algorithms, as Laplace, Gauss or Escobal methods, give very poor results. The present work faces with the problem of estimating the orbital parameters of an orbiting object using its optical streak acquired by a telescope or a high accuracy camera. In the paper a new technique is developed for the Initial Orbit Determination from optical data by exploiting the genetic algorithms. The algorithm works without restrictions on the observer location. A recent challenging problem is the Initial Orbit Determination with space-based observations. This work focuses on the problem of determinating the orbital parameters of a satellite from an orbiting observer in LEO, using short time observations. We present the results based on a simulation with the observer on a sun-synchronous orbit with a single observation of just 60 s. Monte Carlo simulations are presented with different levels of sensor accuracy to show the reliability of the algorithm. The algorithm is able to yield a candidate solution for each observation. The coplanar case is analyzed and discussed as well.     

碳纤维表面CVD硅涂层对其性能的影响

 分析了碳纤维表面化学气相沉积Ｓｉ涂层的相结构,研究了Ｓｉ涂层对碳纤维抗氧化性能及强度的影响。结果表明：涂层中Ｓｉ元素呈非晶态分布；Ｓｉ涂层可提高碳纤维的抗氧化性能；氧化温度不同,Ｓｉ涂层碳纤维的氧化失重或增重规律也不相同。同时,Ｓｉ涂层降低了碳纤维拉伸强度,而适度空气氧化又可使Ｓｉ涂层碳纤维强度得到大幅度提高；Ｓｉ涂层碳纤维的强度随氧化温度、氧化时间的变化而改变。