武器装备费用确定方法及效费比分析探讨

分析了武器装备的全寿命周期费用的构成及特点,提出用装各经济寿命分析的方法计算出装备的全寿命费用;分析了效能费用的辩证关系,对效费比计算进行了初步的探讨。     

远程测发控系统在无人值守期间对部分故障的远程定位

首先要建立模拟量与数字量被合理分配、灵活应用的测控体制,然后再 开始解决一些目前无法进行远程处理的问题;选择一款有助于实现总体方案的 高可靠性数模设备也是设计之初重点考虑的问题。     

Integration of high-fidelity model of forward variable area bypass injector into zero-dimensional variable cycle engine model

Forward Variable Area Bypass Injector (FVABI) is one of key components which contributes to modulate the cycle parameters of Variable Cycle Engine (VCE) under various operation conditions. The modeling method of zero-dimensional FVABI was reviewed and its deficiency was analyzed based on FVABI flow characteristic. In order to improve the accuracy of VCE performance simulation, the high-fidelity modeling method of FVABI was developed based on its working characteristics. Then it was coupled with the zero-dimensional VCE model and the multi-level VCE model was built. The results indicate that the geometric and aerodynamic parameters can affect the interaction between the two airflows and the zero-dimensional FVABI model is too simple to predict the component performance accurately, especially when the FVABI inner bypass is chocked. Based on the performance curves for single bypass mode and the regression model of multi-scale support vector regression for double bypass mode, the high-fidelity model can predict FVABI performance accurately and rapidly. The integration of high-fidelity FVABI model into zero-dimensional VCE model can be done by adjusting iterative variables and balance equations. The multi-level model has good convergence and it can predict VCE performance when the FVABI inner bypass is chocked.     

利用相似周方法预测第24活动周开始时间

利用相似周方法对第24活动周的开始时间与第23活动周下降相后期的太阳黑子数进行了预报.根据第23周已经出现的特征参量和下降相的形态特征,选取9,10,11,15,17和20等六个太阳活动周作为第23周下降相的相似周,对第24周开始时间进行预报.预报结果显示,第24活动周的开始时间为2007年5±1月,黑子数平滑月均极小值为7.1±2.6,第23太阳活动周长度为11.1年.与其他研究者的预报结果相比较,本文给出的结果与文献[11]和[12]及MSFC的结果比较一致.通过对相似周方法在下降相预测太阳活动周结束时间的研究讨论,及对第23周上升阶段的太阳黑子数和F10.7平滑月均值预报结果的评估,可以看出,相似周预报方法在太阳活动周长期预报中是很有应用价值的.      

一种基于自测试的卫星快检技术研究

传统卫星设计以功能实现为主，可测试性较低，卫星综合测试基本依赖遥测遥控，测试周期长、效率低、成本高，不能很好地适应未来卫星批量化研制需求。参考民用汽车快速电检技术，从卫星可测试性与自测试设计出发，设计了基于总线调度的卫星快检系统，提高了卫星快速检修与快速发射能力，满足未来卫星低成本高效率研制需求。     

Comparison of convergence time and positioning accuracy among BDS,GPS and BDS/GPS precise point positioning with ambiguity resolution

Precise point positioning (PPP) usually takes about 30?min to obtain centimetre-level accuracy, which greatly limits its application. To address the drawbacks of convergence speed and positioning accuracy, we develop a PPP model with integrated GPS and BDS observations. Based on the method, stations with global coverage are selected to estimate the fractional cycle bias (FCB) of GPS and BDS. The short-term and long-term time series of wide-lane (WL) FCB, and the single day change of narrow-lane (NL) FCB are analysed. It is found that the range of GPS and BDS non-GEO (IGSO and MEO) WL FCB is stable at up to a 30-day-time frame. At times frame of up to 60?days, the stability is reduced a lot. Whether for short-term or long-term, the changes in the BDS GEO WL FCB are large. Moreover, BDS FCB sometimes undergoes a sudden jump. Besides, 17 and 10 stations were used respectively to investigate the convergence speed and positioning errors with six strategies: BDS ambiguity-float PPP (Bfloat), GPS ambiguity-float PPP (Gfloat), BDS/GPS ambiguity-float PPP (BGfloat), BDS ambiguity-fixed PPP (Bfix), GPS ambiguity-fixed (Gfix), and BDS/GPS ambiguity-fixed (BGfix). The average convergence speed of the ambiguity-fixed solution is greatly improved compared with the ambiguity-float solution. In terms of the average convergence time, the Bfloat is the longest and the BGfix is the shortest among these six strategies. Whether for ambiguity-float PPP or ambiguity-fixed PPP, the convergence reduction time in three directions for the combined system is the largest compared with the single BDS. The average RMS value of the Bfix in three directions (easting (E), northing (N), and up (U)) are 2.0?cm, 1.5?cm, and 5.9?cm respectively, while those of the Gfix are 0.8?cm, 0.5?cm, and 1.7?cm. Compared with single system, the BDS/GPS combined ambiguity-fixed system (BGfix) has the fastest convergence speed and the highest accuracy, with average RMS as 0.7?cm, 0.5?cm, and 1.9?cm for the E, N, U components, respectively.     

采用MSCMG群的卫星平台敏捷机动控制地面闭环试验验证

针对新型惯性执行机构磁悬浮控制力矩陀螺(Magnetically suspended control moment gyro, MSCMG),基于金字塔构型开展卫星平台敏捷机动控制地面闭环试验研究,以验证MSCMG的姿态控制性能。首先基于MSCMG搭建卫星平台控制地面试验系统,建立数学模型;接着针对气浮台外界扰动抑制及大角度敏捷机动控制问题,基于变参数滑模控制设计姿态控制算法,采用鲁棒伪逆方法进行MSCMG群框架角速度分配;并针对MSCMG的特性对框架角速度和角加速度进行了限幅,开展闭环控制试验研究。试验结果表明,采用MSCMG进行气浮台姿态稳定控制实验,可以实现姿态稳定度优于5×10~(-4)(°)/s,且在实现30°/15 s的机动指标时,MSCMG框架角速度具有良好的跟踪性能,且磁悬浮转子在输出大力矩时仍然保持稳定悬浮,具有较强的鲁棒性。通过地面闭环试验验证了MSCMG作为姿控执行机构的优异性能,为其未来进一步应用研究奠定基础。     

Simulation study of motion of charged particles trapped in Earth’s magnetosphere

This article aims to understand the motion of the charged particles trapped in the Earth’s inner magnetosphere. The emphasis is on identifying the numerical scheme, which is appropriate to characterize the trajectories of the charged particles of different energies that enter the Earth’s magnetosphere and get trap along the magnetic field lines. These particles perform three different periodic motions, namely: gyration, bounce, and azimuthal drift. However, often, the gyration of the particle is ignored, and only the guiding center of the particle is traced to reduce the computational time. It is because the simulation of all three motions (gyro, bounce, and drift) together needed a robust numerical scheme, which has less numerical dissipation. We have developed a three-dimensional test particle simulation model in which the relativistic equation of motion is solved numerically using the fourth and sixth-order Runge-Kutta methods. The stability of the simulation model is verified by checking the conservation of total kinetic energy and adiabatic invariants linked with each type of motion. We found that the sixth-order Runge-Kutta method is suitable to trace the complete trajectories of both proton and electron of a wide energy range, 5 keV to 250 MeV for L = 2 – 6. We have estimated the bounce and drift periods from the simulations, and they are found to be in good agreement with the theory. The study implies that a simulation model with sixth-order Runge-Kutta method can be applied to the time-vary, non-analytical form of magnetic configuration in future studies to understand the dynamics of charged particles trapped in Earth’s magnetosphere.     

二阶n次多项式自治系统的极限环的唯一性

主要利用文［１］中的变换，将下列二阶ｎ次多项式自治系统ｄｘｄｔ＝ｇ１（ｘ）＋ｈ１（ｘ）ｙｄｙｄｔ＝ｇ２（ｘ）＋ｈ２（ｘ）ｙ（＊）（其中，ｇ１（ｘ）＝∑ｎｉ＝０ａｉｘｉ，ｈ１（ｘ）＝∑ｎ－１ｉ＝０ｂｉｘｉ，ｇ２（ｘ）＝∑ｎｉ＝０ｃｉｘｉ，ｈ２（ｘ）＝∑ｎ－１ｉ＝０ｄｉｘｉ）变换成Ｌｉｅｎａｒｄ方程，再利用构造Ｄｕｌａｃ函数的方法和文［２］中的一个定理，得到了二阶ｎ次多项式自治系统（＊）的极限环唯一性的几个充分条件。     

Planetary Radiation Budgets

The energy state of a planet depends fundamentally on its radiation budget. Measurements made from space over past decades have led to significant revisions of ground-based estimates, both of the reflected fraction (the Bond albedo) of solar radiative flux and of the emitted thermal infrared radiation flux, for the Earth as well as for the other planets. After a brief survey of methods and difficulties in accurately determining planetary radiation budgets, we note contradictions in existing tabulations of global parameters, in particular Bond albedo. For the Earth, such contradictions are unjustified, considering that global and annual means as well as the seasonal cycle of Earth Radiation Budget components have now been determined with high accuracy. The Earth's Bond albedo is close to 0.3. Net storage of energy in the Earth-ocean system is close to zero, with a well-established annual cycle of amplitude close to ±12 Wm⁻². Some contradictions remain for the other terrestrial planets. For the giant planets, modern reduced values of the Bond albedo imply reduced but still significant internal energy generation.