航管信息GPS时统系统

介绍航管信息 GPS时统系统的开发。描述系统方案设计、基于消息的异步存取技术、多线程技术和网络进程间通信技术 ,重点介绍了系统的开发技巧。     

Spacecraft optimal rendezvous controller design using simulated annealing

A new global approach for rendezvous Linear Quadratic controller design is presented in this paper. Instead of solving the algebraic Riccati equation, a continuous simulated annealing (SA) algorithm is used to design rendezvous LQ controller. Optimization of one automatic rendezvous controller with 18 design parameters is illustrated. The results show that the SA algorithm can locate the global solution effectively and robust, besides a great number of global solutions have been obtained by the SA. The SA has demonstrated better performance than other optimization algorithms such as floating-coded Genetic Algorithm, Simplex method and Powell algorithm.     

温度垂直递减率对飞机尾涡影响的数值模拟

为了更深入精确地研究航空器尾涡演变规律,保障航空器安全运行,本文采用数值模拟方法对不同温度垂直递减率下A330-300飞机尾流的耗散规律进行了研究。数值模拟选择SST (Shear stress transport) k-ω湍流模型,通过构建5种不同温度垂直递减率下的温度场,并在温度场内编译A330-300飞机尾流场实现不同温度垂直递减率下的演化。通过数值模拟结果与雷达探测数据的对比验证了数值模拟方法可靠性。计算结果表明,一般湍流强度下,不同的温度垂直递减率主要作用于尾涡衰减阶段,通过改变尾涡内外温度影响尾涡演化。温度垂直递减率越小,尾涡衰减区环量减小得越快;温度垂直递减率越大,尾涡下沉的速率越大,快速耗散后的涡核间距越大。     

Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

旋成体零攻角纵向大扰动势流的AF-2迭代及其并行算法

 <正> 1.引言 为提高跨音速差分计算效率,人们在计算格式的设计、改进方面做了大量的工作,并取得了可喜的成就。并行计算机的出现和发展,使我们有可能进一步提高计算效率。第9期阂赛金等:旋成体零攻角纵向大扰动势流的人F一2迭代及其并行算法A弓n因为并行处理机具有处理数据能力强、计算效益高的特点,但这种机器必须结合具体问题和机器特点加以考虑才能发挥其优势。目前,利用我国设计的“YH一1”(“银河一1”)亿次并行处理机,开展跨音速差分计算的并行算法研究具有理论和运用上的重要意义     

排队论的局限与排队模拟的数学本质

排队现象是工程技术和社会生活中广泛存在的一种现象。对它进行量的研究将有助于通信、计算机、航天和电子对抗领域一大类问题的解决。排队论［１］为此己做出了重要贡献,但有局限。排队模拟可克服这些局限,提出了排队系统的新定义;对排队论己有成果进行了回顾和分析;指出用Ｌｉｎｄｌｅｙ定理验证非泊松到达的等待时间｛Ｗｎ｝的分布函数之所以十分困难的原因;提出排队论的三点局限;分析了排队模拟的数学本质;指出排队模拟实际上是数列环上的运算。     

等速上仰翼型绕流结构的数值模拟

通过数值求解涡量-流函数形式的N-S方程研究等速上仰翼型的分离流动结构。用ADI方法解涡量方程;用Poisson方程直接法解流函数方程。在计算得到的流场中除可看到实验中观察到的多涡结构外,还发现一些实验中未观察到的现象。将分离流动结构的计算结果与翼型气动力变化相联系,并结合涡动力学理论,定性地解释了上仰翼型产生高升力的原因。     

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.     

椭圆轨道非线性相对运动模型的周期解与应用

在长期的航天器编队飞行中传统的基于线性相对运动模型设计编队保持轨道的方法会引起较多的燃料消耗.首先采用摄动法解析地求得了考虑二阶非线性项时椭圆轨道相对运动模型的周期性条件和周期解;然后以此周期解为参考轨道设计了基于Lyapunov稳定的PD保持控制律.仿真结果表明:基于椭圆轨道非线性相对运动模型的周期解较基于椭圆轨道线性相对运动模型的周期解,精度明显提高;以前者为参考轨道的保持控制与以后者为参考轨道的保持控制相比,燃耗明显降低.     

辅助平面法评定平面对平面倾斜度误差的数学模型

提出一种评定平面对平面倾斜度误差的新算法。该算法是通过确定辅助测量平面，在不含原理误差的条件下，快速、准确地确定符合其定义的倾斜度误差值。