多位数频标测量系统

介绍一种非整数(多位数)频标频率测量系统的工作原理、误差分析及主要技术指标。频率测量范围从1～80MHz,系统的不确定度α<5×10~(-11)/s。该系统还可以同时进行多台频标的自动测试(配上计算机和多路射频开关)。     

编队飞行卫星群构型保持及初始化

导出了基于相对轨道要素的编队飞行卫星群轨道相对运动控制的轨道机动方程；提出了编队飞行卫星群轨道相对运动控制的轨道机动控制策略，利用不同方向的脉冲控制相对运动的轨道参数，包括轨道平面内机动和轨道平面外机动控制。根据相对轨道要素的变轨机动控制，进行编队飞行卫星群构型的初始化。这样的构型初始化可以视作一次特殊的变轨机动控制，很容易实现编队飞行构型的初始化机动。     

平台摇摆对卡尔曼滤波跟踪精度的影响

通过建立目标相对运动坐标系和目标相对运动观测模型,研究了在平台摇摆影响下,跟踪系统观测到的目标运动状态的变化。在分析捷联垂直基准补偿原理的基础上建立了捷联垂直基准平台摇摆角补偿模型,建立的模型结合捷联垂直基准系统的测量能力对其补偿算法进行了理论推导,使模型适用于实际捷联垂直基准系统。通过建立模型以及仿真研究了平台摇摆作用下卡尔曼滤波跟踪精度的变化,指出了摆造成卡尔曼滤波跟踪精度降低甚至离散的主要原因在于模型误差增大。设计仿真实验验证了结论的正确性,为进一步改进跟踪手段提供了理论参考。     

Coupled Stress-Electricity Model for Electromagnetic Emission Induced by Concrete Fracture

Electromagnetic emission induced during concrete fracturing is of great significance to health monitoring of concrete structures.A coupled stress-electricity model is established by analyzing the interaction between stress and electricity during concrete fracturing.And based on this model,the electromagnetic radiation parameters are calculated.The theoretical calculation is well coincident with experimental results.This work provides theoretical support for concrete testing system.     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.     

球阀阀座用聚三氟氯乙烯密封环工艺与性能

选用两种不同降温方式探究压制成型工艺对球阀阀座用聚三氟氯乙烯（PCTFE）密封环密封性能的影响。低温试验结果表明,自然降温工艺成型的制品外表面在常温-低温循环工况下出现裂纹,而保压降温得到的制品则不出现上述问题。性能测试与表征分析结果表明,自然降温工艺成型的密封环PCTFE其内部会出现微裂纹等缺陷,导致其在低温测试后出现亚表面裂纹,造成密封失效。降温阶段保压操作可抑制材料成型阶段微裂纹缺陷的产生,避免材料在室温-低温循环工况下因内应力而产生裂纹缺陷。     

流场可压缩性对涡相互作用影响的数值研究

涡相互作用作为冲压发动机喷注装置的典型抽象流动现象,研究其可压缩性影响对于认识包含化学反应的真实燃料喷射场具有一定基础理论价值。基于经过数值验证的可压缩Navier-Stokes算法与压力泊松方程初始条件设置方法研究流场可压缩性对涡相互作用演化过程的影响。结果表明,以较高涡旋马赫数表征的可压缩性在改变涡对形态的同时,具有延缓涡旋相互靠近,迟滞融合进程的作用。关于涡对系统开始融合的临界条件,可压缩相互作用开始的临界展弦比与无量纲时间相比于低速涡对明显提高。为在无量纲时间意义下统一不同马赫数涡对相互作用的进程,从涡心密度随时间变化规律出发在不可压涡对特征时间的基础上,初步构建了考虑可压缩性的时间尺度修正关系。     

储氢合金的性质及发展趋势

本文介绍了储氢合金的性质，Ｎｉ－ＭＨ电池原理，以及储氢合金对Ｎｉ－ＭＨ电池所产生的影响，根据目前科学技术的发展以及市场的需求，提出了未来储氢合金及Ｎｉ－ＭＨ电池的发展趋势。     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.