电脑控制磁粉探伤机的研制

本文介绍了利用ＭＣＳ－５１单片机进行磁化参数与操作功能控制的磁粉探伤的工作原理，特点及技术性能。该机经民航，汽车等知业检验部门的使用效果良好。     

隐马尔可夫模型在对象定位中的应用与实现

以医学图像中脊柱的定位为应用背景,对经典Viterbi算法进行改进,根据全局最优搜索算法提出了可控的最优搜索算法,把隐马尔可夫模型(Hidden Markov model,HMM)应用于二维图像中线性结构对象的定位。以真实的人体脊柱X光照片为实验样本进行的定位实验,结果表明:HMM模型不需要对图像施加较多的限制,就可获得较成功的定位结果,同时引入了可控的最优搜索算法后,定位效果有了进一步的提高。还通过实验分析了可控制的最优搜索的两个控制参数对定位性能的影响,并提出了定位性能具有区间性的结论。     

淮北地区水稻适宜发展规模的研究

准北地区水稻发展的主要制约因素是水资源，该地区水资源系统是江水北调大系统的一个有机部分，其水稻适宜规模取决于江水北调系统水资源的开发利用。根据输水线路或水资源特征将整个系统划分为１５个子系统，以水资源利用量最大，以及缺水造成的减产损失和提水费用之和最小作为水资源利用的两个目标，建立了模拟分析数学模型，提出了求解该模型的大系统分解一协调技术，给出了模拟模型的执行顺序和运行程序，研究了当前工程水平、泵站改造项目完成、通榆河工程完成和南水北调工程建成四种情况淮北水稻适宜发展规模。     

大型火箭振动试验振型斜率测试方法

讨论了在火箭固有振动频率下测量振型斜率的几种计算和测试方法，分析了影响振型斜率测量和符号误判的误差源，提出了按秒状态变化进行振型斜率修正的最小二乘曲线拟合法。研究表明，以参照点陀螺信号为基准计算相位角，可以避免相位符号的误判。这一改进对于以相位符号作为稳定性判别准则的控制系统来说是至关重要的。     

飞行控制系统实物在回路中的仿真

５０年代末，南京航天航天大学就开始研究仿真技术工作，并研制成功包括三自由度液压飞行模拟转台在内的若干专用模拟器。在这套仿真设备上，圆地完成了多种型号无人驾驶飞机、导弹、舰船控制系统地面仿真试验。本文简要地介绍这套设备的技术性能，以及系统仿真在飞行控制系统研制过程中不同阶段的应用效果。     

飞行仿真转台混合灵敏度设计

以ET－ⅢA型电动伺服转台为背景，在分析了转台系统的不确定性及其性能指标要求的基础上，利用H∞混合灵敏度方法对转台系统速度环进行了设计，并通过计算机实现控制算法，最终的调试结果满足系统的性能要求，从而验证了设计方法的可行性和有效性。     

差分流量调节推力矢量控制研究

为了了解差分流量调节实现推力矢量控制的特点,参考塞式喷管发动机XRS 2200的工作参数,对多单元直排型塞式喷管模型发动机进行了数值计算。介绍了差分流量调节的计算方法和内喷管与塞锥推力矢量变化的分析过程,计算产生的俯仰力矩。结果表明,差分流量调节时,塞式喷管轴向合力基本保持不变,不损失轴向推力性能;俯仰力矩包括轴向力和侧向力产生的两部分力矩,随差分流量调节增大而增加,有很好的偏转性能。结论可以为差分流量调节的实验研究提供参考。     

Biaxial Mode of Rotation of a Satellite in the Orbit Plane

A mode of motion of a satellite with respect to its center of mass is studied, which is called the biaxial rotation in the orbit plane. In this mode of rotation, an elongated and nearly dynamically symmetric satellite rotates around the longitudinal axis, which, in turn, rotates around the normal to the plane of an orbit; the angular velocity of rotation around the longitudinal axis is several times larger than the orbital angular velocity, deviations of this axis from the orbit plane are small. Such a rotation is convenient in the case when it is required to secure a sufficiently uniform illumination of the satellite's surface by the Sun at a comparatively small angular velocity of the satellite. The investigation consists of the numerical integration of equations of the satellite's motion, which take into account gravitational and restoring aerodynamic moments, as well as the evolution of the orbit. At high orbits, the mode of the biaxial rotation is conserved for an appreciable length of time, and at low orbits it is destroyed due to the impact of the aerodynamic moment. The orbit altitudes and the method of constructing the initial conditions of motion that guarantee a sufficiently prolonged period of existence of this mode are specified.     

铅化合物在双基推进剂燃烧过程的作用机理

本文提出了铅化合物催化双基推进剂燃烧的反应历程。充分说明这类化合物是最终通过提高燃烧表面处嘶嘶区温度梯度提高燃速的。本文还提出了“铅化合物有通过增加燃烧表面上碳质物量增加燃速的一面,还有通过减少碳质物抑制燃速增加的一面”这一新的论点及抑制碳质物增加的反应并阐明了压力对这种抑制能力的影响。最后根据本文提出的作用机理及传热原理圆满解释了超速、平平和/或麦撒效应。     

Statistical Relationships between Solar,Interplanetary, and Geomagnetic Disturbances, 1976–2000: 3

In this paper we continue the analysis of the influence of solar and interplanetary events on magnetic storms of the Earth that was started in [9, 10]. Different experimental results on solar-terrestrial physics are analyzed in the study and the effects are determined that arise due to differences in the methods used to analyze the data. The classifications of magnetic storms by the K _p and D _st indices, the solar flare classifications by optical and X-ray observations, and the classifications of different geoeffective interplanetary events are compared and discussed. It is demonstrated that quantitative estimations of the relationships between two types of events often depend on the direction in which the events are compared. In particular, it was demonstrated that the geoeffectiveness of halo CMEs (that is, the percentage of Earth-directed coronal mass ejections that result in geomagnetic storms) is 40–50%. Higher values given in some papers were obtained by another method, in which they were defined as the probability of finding candidates for a source of geomagnetic storms among CMEs, and, strictly speaking, these values are not true estimates of the geoeffectiveness. The latter results are also in contrast with the results of the two-stage tracing of the events: first a storm—an interplanetary disturbance, and then an interplanetary disturbance—a CME.