高能氧化剂二硝酰胺铵的热分解研究

为深入了解二硝酰胺铵(ADN)的热分解，为该氧化剂在推进剂中应用提供必要的技术保障和实验依据，采用热重分析法(TG)及差示扫描量热法(DSC)，实验研究了氮气流量、合成中间体烷基羰基N-硝酰胺铵(AUN)及硝酸铵(AN)对ADN热分解过程的影响，并利用model-free isoconversional方法模ADN热分解过程的活化能曲线。结果表明：氮气流量和硝酸铵(AN)对ADN的热分解过程有显著影响，而AUN可使ADN热分解曲线产生肩峰，但基本不影响ADN的热分解过程。     

变频信号的测量方法

本文阐述了单片机测量车用电子警报器变频信号的原理和方法。     

热冲击再时效对Al—Zn—Mg—Cu合金组织及性能的影响

用高压电子显微镜对LC4-CS合金进行不同温度下的高温同位组织观察,证明该合金的晶间析出和基体沉淀可以同时固定在时效沉淀序列的不同阶段,使晶间呈过时效状态,而基体组织处于峰值时效状态。通过本文提出的热冲击再时效工艺方法可以获得以上组织状态,从而达到高强度铝合金主要性能的最佳组合。     

一种新颖的瞬时浮点放大器

介绍了瞬时浮点放大器的原理及构成，并给出一种结构新的具有２５６阶的瞬时浮点放大器，可有效地提高数据采集系统的测量范围。     

悬索桥颤振主动抑制研究

选用二次型性能指标，把悬索桥颤振主动抑制问题转化为线性二次型高斯问题，设计了颤振主动抑制的最优滤波器及最优控制律，其中，经ｏｇｅｒ有理近似拟合气动力自激项，对脉动风的描亭旭结为成型滤波器设计；稳定性判定归结为根轨迹图的判断；抖振响应计算归结为Ｌｙａｐｕｎｏｖ方程求解，以某悬索桥为算例，计算结果表明：对该类桥梁进行颤振主动抑制，效果良好，最优控制设计所得结论对工程具有一定参考价值。     

非线性随机动态系统学习建模方法

在动态神经网络及扩展卡尔曼滤波算法的基础上，提出了对非线性随机动态系统进行学习建模的迭代算法，用这种方法对非线性随机系统建模，可以获得更准确伯系统模型，并可对非线性随机系统进行状态估计。最后给出相应算法及仿真结果。     

Early analysis of precise orbit and clock offset determination for the satellites of the global BeiDou-3 system

Eight new-generation BeiDou satellites (BeiDou-3) have been launched into Medium Earth Orbit (MEO), allowing for global coverage since March 2018, and they are equipped with new hydrogen atomic clocks and updated rubidium clocks. Firstly, we analyzed the signals for the carrier-to-noise-density ratio (C/N0) and pseudorange multipath (MP) by using international GNSS (Global Navigation Satellite System) Monitoring and Assessment System (iGMAS) station data, and found that B1C has a lower C/N0, and B2a has the same level of C/N0 as the B1I and B3I signals. For pseudorange multipath, compared with the BeiDou-2 satellites, the obvious systematic variation of MP scatters related to the elevation angle is greatly improved for the BeiDou-3 and BeiDou-3e satellites signals. For the signals of the BeiDou-3 satellites, the order of the Root Mean Square (RMS) values of multipath and noise is B3I?<?B1I?<?B2a?<?B1C. Then, the comparison of the precise orbit determination and clock offset determination for the BeiDou-2, BeiDou-3, and BeiDou-3 experimental (BeiDou-3e) satellites was done by using 10 stations from iGMAS. The 3D precision of the 24?h orbit overlap is 24.55, 25.61, and 23.35?cm for the BeiDou-3, BeiDou-3e, and BeiDou-2 satellites, respectively. BeiDou-3 satellite has a comparable precision to that of the BeiDou-2 satellite. For the precision of clock offset estimation, the Standard Deviation (STD) of the BeiDou-3 MEO satellite is 0.350?ns, which is an improvement of 0.042?ns over that of the BeiDou-2 MEO satellite. The stabilities of the BeiDou-3 and BeiDou-3e onboard clocks are better than those of BeiDou-2 by factors of 2.84 and 1.61 at an averaging time of 1000 and 10,000?s, respectively.     

Very Long Baseline Interferometry: Dependencies on Frequency Stability

Very Long Baseline Interferometry (VLBI) is a differential technique observing radiation of compact extra-galactic radio sources with pairs of radio telescopes. For these observations, the frequency standards at the telescopes need to have very high stability. In this article we discuss why this is, and we investigate exactly how precise the frequency standards need to be. Four areas where good clock performance is needed are considered: coherence, geodetic parameter estimation, correlator synchronization, and UT1 determination. We show that in order to ensure the highest accuracy of VLBI, stability similar to that of a hydrogen maser is needed for time-scales up to a few hours. In the article, we are considering both traditional VLBI where extra-galactic radio sources are observed, as well as observation of man-made artificial radio sources emitted by satellites or spacecrafts.     

Evaluation of the Terrestrial Albedo Applied to Some Scientific Missions

Using the Earth albedo model and the orbital dynamics model developed as part of the First Look Project (Fast Initial In-Orbit Identification of Scientific Satellites) the terrestrial albedo is evaluated considering the orbits of some scientific missions as Gravity Probe B, MICROSCOPE and STEP. The model of the Earth albedo is based on the reflectivity data measured by NASA’s Earth Probe satellite, which is part of the TOMS project (Total Ozone Mapping Spectrometer). The reflectivity data are available daily, on line at the TOMS website, and they fluctuate because of changes in clouds and ice coverage and seasonal changes. The data resolution partitions the Earth surface into a number of cells. The incident irradiance on each cell is used to calculate total radiant flux from the cell. With the radiant flux from each cell, the irradiance at the satellite is calculated.