eLoran系统ASF网格应用算法研究

ASF网格是提高增强型罗兰（Enhanced Long Range Navigation,eLoran）系统精度的重要方法。根据所在网格四个顶点的附加二次时延（Added Secondary Factor,ASF）值通过网格应用算法得到待测试点的ASF值,一定程度上比公式计算的ASF值更准确。在计算过程中,用户四个顶点ASF值的测量误差会传递给用户,同时内插算法本身也会引入误差,此时内插算法的选择尤为重要。本文通过仿真、分析比较几种常用的内插算法,得出结论：反距离插值算法引入的误差最大,双线应插值算法引入的误差最小,而且误差呈现一定层次感,网格从内到外误差逐渐减小。     

多航天器协同探测效能影响参数不确定性分析

为解决传统基于蒙特卡洛仿真的探测效能不确定性分析评价方法中时间效率低,参数关系映射单一的问题,提出一种基于神经网络的不确定性分析方法,利用人工神经网络在拟合回归分析上的非线性特性,设计了能够替代复杂系统的神经网络结构,能够通过少量仿真计算结果作为训练样本实现模型的收敛并能有效反映被替代系统的原有特性。选择以一个多航天器的天文观测任务作为典型用例,建立了仿真分析模型,并与蒙特卡洛仿真方法结果进行了对比,验证了此方法的准确性和计算效率。     

Radio Occultation Measurements of the Radio Wave Absorption and the Sulfuric Acid Vapor Content in the Atmosphere of Venus

The results of the determination of centimeter ( = 5 cm) radio waves absorption in the radio occultation experiments, carried out using the Venera-15and Venera-16spacecraft, are presented. The altitude distribution of the absorber substance is analyzed. The absorbing layer is shown to exist at altitudes of 64 to 58 km in the near-polar regions of the planet. At middle latitudes such an absorbing layer was not found. In the altitude range from 56 to 46 km the radio wave absorption by the sulfuric acid (H₂SO₄) vapor is observed. The content of the sulfuric acid vapor is shown to increase with decreasing altitude: in the mid-latitude region at altitudes of 56.7 and 53 km it equals 5 and 20 ppm, respectively, and at polar latitudes the same content of H₂SO₄vapor is observed at altitudes of 51.2 and 47 km, respectively. A comparison of these results with the data of radio wave absorption in the = 13 cm band, obtained in the Pioneer Venus Orbiterradio occultation experiments, leads to the conclusion that the obtained values of the sulfuric acid vapor content well agree in the regions of overlap of the data.     

试飞测试数据的数据特性分析

提出利用小波变换的多分辨率特性 ,对安装在飞机机翼上的应变传感器的实测数据进行分析 ,得出其频率特性。并将该方法与传统快速傅立叶变换分析结果进行比较 ,探讨了使用小波变换对工程实测数据进行分析的可行性。     

Airglow in the Visible and Infrared Spectral Ranges of the Disturbed Upper Atmosphere under Conditions of High-Velocity Plasma Jet Injection: I. Experimental data

The measurements of infrared emission from an artificial structure, which was generated during the Fluxus experiment with plasma jet injection into the atmosphere, are obtained and discussed for the first time. Additional experimental data on the airglow in the visible spectral band of the disturbed region of the atmosphere are presented. A generalized analysis of the data is given.     

航天测控与数传接收综合信道构想

提出 S/ X航天测控与数传接收综合信道的概念 ,对综合信道进行了设计 ,重点说明综合信道中伪码测距的实现方法。讨论设计测控系统和应用系统综合信道的三种方案 ,并进行了比较分析。     

扩展旋转矢量捷联姿态算法

给出了一种新的旋转矢量捷联姿态构造算法，该算法由陀螺样本的多重积分来构造旋转矢量的最小二乘估计。新算法具有较好的顺序递推结构，易于在机载计算机上编程实现，比传统方法更容易满足一些限制较多的特殊应用。文中还给出了该算法在机载计算机上的计算流程及算法的局部硬件化实现。     

运载火箭发射过程效能评估方法研究

论述了效能评估模型及一般分析方法 ,确定了定量和定性分析相结合的运载火箭发射过程评估方案 ,阐述了运载火箭发射过程效能评估的多指标综合评价方法 ,应用层次分析法建立了评估模型 ,规划了评估体系。论文最后给出的部分仿真结果描述了系统总体效能和设施设备工作情况及重要度之间的关系 ,这种关系是符合工程实际的。     

Determination of the Microacceleration Quasisteady Component onboard the International Space Station

A comparison of two methods of determination of the microacceleration quasisteady component arising onboard the International Space Station was performed. In the first method the acceleration was calculated using the relative motion of the station reconstructed on the basis of telemetry data. The second method was a direct measurement of the microacceleration by a low-frequency accelerometer and a smoothing of the data obtained. The used measurements were made by the American accelerometer MAMS. The above comparison can theoretically be used to refine the position of the station center of mass relative to its body.     

气动塞式喷管底部压强模型研究

为了解塞式喷管底部压强特点,找出快速、准确计算底部压强的方法,实验研究了不同反压下塞式喷管的底部压强.在认识外界反压对塞式喷管流动作用机理的基础上分析如何确定不同的底部气动状态,将塞式喷管底部在不同外界反压下的气动状态划分为"三段",即底部开放段、底部闭合段和底部由开到闭的过渡段,在各段,底部压强使用不同的计算方法.把数值模拟、实验研究及塞式喷管底部自身特点结合起来,找出塞式喷管底部压强的一般规律,建立了适合于工程应用的底部压强计算模型.结合40%和20%截短塞式喷管的实验数据,验证了底部模型的正确性.塞式喷管底部流动是超声速流的大分离流动,该模型对底部压强的预示比有限差分法具有更高的精度.