含纳米金属粉的推进剂点火实验及燃烧性能研究

利用CO2激光点火系统对含有纳米铝粉和纳米镍粉的AP／HTPB推进剂进行激光点火实验,测量了推进剂在不同激光功率和压强下的点火延迟时间,对推进剂的燃速、常压点火温度和爆热也进行了测量。同时,利用氧化还原滴定法测定燃烧残渣中活性铝含量。结果表明,纳米铝粉(n—Al)的点火阀值比普通铝粉(g-A1)的点火阀值小几个数量级,加入纳米铝粉可有效地缩短推进剂点火延迟时间。而在纳米镍粉为催化剂的协同作用下,推进剂燃速明显提高,点火延迟时间也大大减少,Al在推进剂燃烧过程中的燃烧效率得以提高,同时燃烧残渣中活性铝含量也明显降低。     

基于FPGA的显控器设计

小巧、坚固耐用的显示器在许多电子设备中得到应用。然而显示控制器为产生多样的显示信息和严格的控制时序,功能复杂且调试困难。本文介绍了一种基于FPGA的显示控制器的设计技术,提出了嵌入仿真模型的调试方法。     

实时微分控制的算法研究

实时微分控制是进行航天器轨道控制的主要方法。本文在费景高所提出的算法基础上 ,提出了一种有效的改进算法 ,扩大了算法的适用范围。文章对算法的稳定性进行了研究 ,并给出了此算法在弹道导弹显式制导中的应用实例。     

掌人心

摘 要 从传统文化角度结合实际分析掌人心的理论和方略。利益诱导人心，教育净化人心，思想文化变换人心和高尚人格诚服人心。     

RDX/AP/HTPB推进剂热分解特性研究

利用高压差示扫描量热仪（PDSC）研究了RDX／AP／HTPB推进剂系列配方的热分解性能，发现配方组分的改变对RDX／AP／HTPB推进剂的热分解性能有影响，突出表现在RDX／AP／HTPB推进剂中RDX分解峰变宽，AP放热分解效应增强。推进剂中添加Al粉后，RDX的分解受到抑制，而AP的分解却得到增强。     

8m×6m 风洞测控处系统

８ｍ×６ｍ风洞测控处系统以ＶＡＸ－Ⅱ为上位机,通过ＱＢＵＳ总线连接数据采集、速压控制、模型姿态角控制和数据实时分析与显示等四个子系统,完成对风洞试验的管理和数据测量与分析及显示。本文介绍了该系统的构成、主要功能和技术指标等。     

Matching suitable feature construction for SAR images based on evolutionary synthesis strategy

In the paper,a set of algorithms to construct synthetic aperture radar（SAR）matching suitable features are frstly proposed based on the evolutionary synthesis strategy.During the process,on the one hand,the indexes of primary matching suitable features（PMSFs）are designed based on the characteristics of image texture,SAR imaging and SAR matching algorithm,which is a process involving expertise;on the other hand,by designing a synthesized operation expression tree based on PMSFs,a much more flexible expression form of synthesized features is built,which greatly expands the construction space.Then,the genetic algorithm-based optimized searching process is employed to search the synthesized matching suitable feature（SMSF）with the highest effciency,largely improving the optimized searching effciency.In addition,the experimental results of the airborne synthetic aperture radar ortho-images of C-band and P-band show that the SMSFs gained via the algorithms can reflect the matching suitability of SAR images accurately and the matching probabilities of selected matching suitable areas of ortho-images could reach 99±0.5%.     

A strategy for investigation of the outer solar system

The requirements of systematic exploration of the outer solar system have been intensively studied by a Science Advisory Group (SAG) of consulting scientists for the National Aeronautics and Space Administration (NASA). Comets and Asteroids were excluded from this study, as a separate group is planning missions to these bodies. This paper and accompanying articles on specific related scientific subjects written by members of the SAG, summarize the findings and recommendations of this group. These recommendations should not be interpreted as official NASA policy. Following some general introductory remarks, a brief sketch is given of the development and current status of scientific missions to the inner planets by the U.S. and the U.S.S.R. With this perspective, the development of the U.S. program for investigation of the outer solar system is described. The scientific focus of outer solar system exploration has been studied in detail. The relationship of the outer planetary bodies to one another and to the inner planets, as parts in a unified solar system evolved from a primitive solar nebula, is emphasized. Deductions from outer solar system investigations regarding the conditions of the solar nebula at the time of planetary formation have been considered. Investigations have been proposed that are relevant to studies of the atmospheric structure and dynamics, internal structure of the planets, satellite composition and morphology, and planetary and interplanetary fields and energetic particles. The mission type and sequence required to conduct a systematic exploration of the outer solar system has been developed. Technological rationales for the suggested missions are discussed in general terms. The existing NASA program for outer solar system exploration is comprised of four missions:

1. Pioneer 10 fly-by mission to Jupiter and beyond, currently underway, with launch on 3 March 1972;
2. Pioneer G, intended for a similar mission with planned launch 2–22 April 1973; and
3. Two Mariner Jupiter/Saturn fly-bys in 1977, with experiment selection scheduled for late 1972 and detailed engineering design during 1972–74.

The Science Advisory Group advocates that detailed mission planning be undertaken on the following additional missions for launches during the late 1970's and early 1980's. Together with existing plans, these would provide a balanced, effective exploration program.

1. 1976 Pioneer Jupiter/Out-of-Ecliptic (One Mission)
2. 1979 Mariner Jupiter/Uranus Fly-bys (Two Missions)
3. 1979 Pioneer Entry Probe to Saturn 1980 Pioneer Entry Probe to Uranus via Saturn Fly-by (Three Missions)
4. 1981/1982 Mariner Jupiter Orbiter (Two Missions).

     

基于多核融合的目标大面积遮挡处理方法

提出了一种基于多核融合的目标遮挡处理方法,用于提高大面积遮挡情况下视觉目标跟踪算法的鲁棒性和准确性.与现有基于单个对称核加权直方图的mean shift跟踪算法不同,该方法以目标区域内的多个非中心位置为核函数中心,构建多个非对称核加权直方图.由于这些直方图对目标的不同区域赋予了不同的权重,使得在遮挡发生时总存在一些直方图受影响较小.依据各个直方图分别进行mean shift迭代获得一组目标位置估计后,利用D-S证据理论融合判定最终的目标位置.实验结果表明,该方法在目标被大面积遮挡时仍能够获得准确的跟踪.