压电陶瓷晶片受迫振动分析及其应用

从基本压电方程出发,推导了压电陶瓷晶片面内受迫振动计算公式,并结合共振实验,提出了一种直接测量压电陶瓷晶片压电常数的方法.与传统的压电常数测量方法相比较,本方法具有许多优点.由于减少了中间环节,测量结果的精度也得到了提高.      

齿向分段抛物线修形对渐开线花键副微动磨损参数的影响

提出渐开线花键副齿向修形的分段抛物线函数,得到齿向修形渐开线花键副的几何模型.使用有限元方法对典型渐开线花键副进行微动摩擦接触分析,得到修形和未修形渐开线花键副的接触应力及相对滑移分布,并考虑修形位置和修形量对齿向修形渐开线花键副微动磨损参数的影响.研究结果表明:分段抛物线函数能满足渐开线花键副的齿向修形要求,修形曲线过渡平滑;齿向修形能有效地减少齿面端部接触应力和相对滑移的集中;典型模型下,修形位置集中在外花键端部和后半段时效果较好;端部修形量应根据模型合理选择, 一般外花键后端的修形量相对前端较大.      

An Investigation of the Mechanical Properties of Some Martian Regolith Simulants with Respect to the Surface Properties at the InSight Mission Landing Site

In support of the InSight mission in which two instruments (the SEIS seismometer and the \(\mbox{HP}^{3}\) heat flow probe) will interact directly with the regolith on the surface of Mars, a series of mechanical tests were conducted on three different regolith simulants to better understand the observations of the physical and mechanical parameters that will be derived from InSight. The mechanical data obtained were also compared to data on terrestrial sands. The density of the regolith strongly influences its mechanical properties, as determined from the data on terrestrial sands. The elastoplastic compression volume changes were investigated through oedometer tests that also provided estimates of possible changes in density with depth. The results of direct shear tests provided values of friction angles that were compared with that of a terrestrial sand, and an extrapolation to lower density provided a friction angle compatible with that estimated from previous observations on the surface of Mars. The importance of the contracting/dilating shear volume changes of sands on the dynamic penetration of the mole was determined, with penetration facilitated by the \(\sim1.3~\mbox{Mg/m}^{3}\) density estimated at the landing site. Seismic velocities, measured by means of piezoelectric bender elements in triaxial specimens submitted to various isotropic confining stresses, show the importance of the confining stress, with lesser influence of density changes under compression. A power law relation of velocity as a function of confining stress with an exponent of 0.3 was identified from the tests, allowing an estimate of the surface seismic velocity of 150 m/s. The effect on the seismic velocity of a 10% proportion of rock in the regolith was also studied. These data will be compared with in situ data measured by InSight after landing.     

高比冲双组元液体远地点火箭发动机研究

综述了国内外研制的双组元液体远地点火箭发动机的性能、特点和发展趋势。在分析了液体远地点发动机提高比冲的各种技术途径后，提出可通过改进喷注器设计、减少边区液膜冷却流量、采用扰流环二次燃烧和使用新型耐更高温材料等措施，以提高远地点发动机的比冲。     

Polarization pattern of low and mid-frequency magnetic pulsations in the polar cap: A comprehensive analysis at Terra Nova Bay (Antarctica)

The polarization pattern of ULF pulsations (f ≈ 1–100 mHz) at Terra Nova Bay (Antarctica, CGM λ ∼ 80°) has been determined for the entire 2003, soon after the solar maximum. A comparison with the results of previous investigations, conducted at the same station close to the solar minimum (1994–96), allows to focus common elements and major differences among different frequency bands which persist through the entire solar cycle. Basically, between f ∼ 1.5 and 5 mHz, the day can be divided into four sectors with alternate polarizations. The local time and latitudinal dependence of the observed pattern can be tentatively interpreted in terms of a latitude of resonant field lines reaching λ ∼ 80° in the noon sector; on the other hand, resonance effects of lower latitude field lines can be clearly identified also far from the noon meridian when the station moves into the deep polar cap. Moreover, in the morning sector the resonance region would extend to lower latitudes than in the evening sector. The proposed profile of the resonant region can interpret also the results obtained at other cusp/auroral stations and appears consistent with that one inferred in the northern hemisphere at smaller latitudes. The resonance region progressively shifts toward lower latitude with increasing frequency; correspondingly, the four-sector pattern progressively disappears at TNB. Above f ∼ 20 mHz, the experimental observations might suggest an additional contribution from Sunward propagating waves, possibly via the magnetotail lobes.     

针对GPS接收机性能的压制干扰区域分析

针对采用扩频增益作为GPS接收机抗干扰容限的非普适性和不确定性,通过建立压制干扰造成GPS接收机不同性能指标下降与分析对象之间的对应关系,将干扰威力区域用受扰区、半失效区和失效区来进行划分。结合GPS接收机工作原理,从理论上推导和分析了在连续波（CW）和宽带高斯噪声干扰下不同相关积分时间的接收机捕获、跟踪和解调等环节的性能下降到临界值时所需干信比。考虑干扰源高度与接收机天线增益的关系,对各威力区的有效干扰距离随干扰源发射功率变化情况进行仿真计算。仿真结果表明,随着干扰功率的提高,干扰源高度对有效干扰距离的影响在逐渐减小。在相同干扰功率下,CW干扰性能要优于宽带高斯噪声干扰。尽管增加接收机相关积分时间会使半失效区和失效区的范围减小,但却会引起受扰区范围显著增大。     

基于PC-BUS的通用可编程A/D转换组件的设计方法探讨

本文介绍了以ＨＡＤＣ５７４２（或ＡＤ１６７４）为核心的基于ＰＣ－ＢＵＳ的通用可编程Ａ／Ｄ转换组件的原理,介绍了Ａ／Ｄ转换组件的设计方法、工作方式、时序分析及其注意事项,对于特殊的可编程Ｉ／Ｏ组件和智能接口卡的设计具有借鉴意义。     

月面热环境的反演研究

以嫦娥三号巡视器月面日食期间非稳态的温度遥测数据为基础,通过建立月壤及巡视器的传热模型,反演了日食期间月面温度的变化,并给出了符合巡视器温度遥测的月壤热物性参数取值范围。在此基础上,对月面热环境进行了分析研究。结果表明,本文反演的月壤平均导热系数大于常见取值,而比热却明显小于常见取值。采用反演的热物性值计算的月表温度与之前认识相符,但对月壤内部热环境有新发现,其温度梯度相对减小而恒温层厚度则明显增大。     

液氧加注过程热力性能分析

为满足某型号运载火箭动力系统试验液氧加注温度要求,需对加注过程进行热力性能分析。通过对常规氧加注过程因漏热和流阻损失引起的温升、液氧泵效率损失引起的温升进行理论计算,得出常规氧加注过程液氧温度变化规律。此外,通过对过冷氧温度掺混特性进行理论计算和数值仿真,得出过冷氧加注的热力性能。上述分析结果与实测数据进行了比对,结果表明,理论分析结果与实测结果吻合性好,液氧加注过程热力特性分析方法正确可行。     

纳米铜铬复合氧化物对RDX热分解的催化作用

为了研究纳米CuO.Cr2O3复合物的催化性能，采用室温固相化学反应法制备出不同铜、铬质量比的纳米CuO.Cr2O3复合物，测出产物的粒径约为15nm，用DSC测试了纳米CuO.Cr2O3复合物对RDX热分解的催化作用。结果表明．：纳米CuO.Cr2O3复合物对RDX热分解有较好的催化效果，它使RDX的分解峰温提前了11．1℃，活化能降低了17kJ/mol，其作用明显优于纳米CuO和纳米Cr2O3及其混合物。