一种三维航迹快速搜索方法

本文提出了基于SAS的自动三维航迹规划方法。该方法通过把约束条件结合到搜索算法中去，有效地减小了搜索空间，缩短了搜索时间，从而使三维规划能够用于实时航迹规划。在搜索过程中地形信息得到了充分利用，使算法生成的航迹能够自动回避地形和威胁。实验证明，该方法能够快速有效地完成规划任务，获得满意的三维航迹。     

动态环境中的飞行器实时三维航迹规划方法研究

本文提出了一种新的飞行器三维航迹规划方法－SDS。该方法能够在具有预先未知威胁的飞行环境中在线实时航迹规划。当飞行器上装备的探测器探测到飞行环境中有预先未知的威胁出现时，根据探测到的信息及时更新威胁数据。SDS根据新的环境信息局部修正受到影响的航迹段来获得新的全局最优航迹。在每一时刻考虑当前已知的信息下，SDS生成的航迹是满足要求的最优航迹。     

EMV规范中的密钥管理

介绍EMV规范的来历和规范中所采用的3DES算法、RSA算法等密码算法的原理。分析两种密钥的生命周期和在EMV规范中的层次结构,同时说明EMV规范对两种密钥的管理方法。     

复合材料机翼翼梁与蒙皮间应力分析

本文采用三维有限元模式，用“ＡＢＡＱＵＳ”分析程序，进行了复合材料机翼翼梁和蒙皮结构的应力分析，对所获得的缘条和蒙皮之间六个应力分量的分布曲线，与采用二维有限元模式的结果做了对比分析，得出了一些有益的结论。     

二维测量系统的误差分析及其修正

二维测量系统的测量误差主要由两个导轨的五个自由度误差和测头误差组成。给出了误差的数学模型，论述了误差的测量、修正及误差修正的误差。     

Plasmaspheric electron content derived from GPS TEC and FORMOSAT-3/COSMIC measurements: Solar minimum condition

The plasmaspheric electron content (PEC) was estimated by comparison of GPS TEC observations and FORMOSAT-3/COSMIC radio occultation measurements at the extended solar minimum of cycle 23/24. Results are retrieved for different seasons (equinoxes and solstices) of the year 2009. COSMIC-derived electron density profiles were integrated up to the height of 700 km in order to retrieve estimates of ionospheric electron content (IEC). Global maps of monthly median values of COSMIC IEC were constructed by use of spherical harmonics expansion. The comparison between two independent measurements was performed by analysis of the global distribution of electron content estimates, as well as by selection specific points corresponded to mid-latitudes of Northern America, Europe, Asia and the Southern Hemisphere. The analysis found that both kinds of observations show rather similar diurnal behavior during all seasons, certainly with GPS TEC estimates larger than corresponded COSMIC IEC values. It was shown that during daytime both GPS TEC and COSMIC IEC values were generally lower at winter than in summer solstice practically over all specific points. The estimates of PEC (h > 700 km) were obtained as a difference between GPS TEC and COSMIC IEC values. Results of comparative study revealed that for mid-latitudinal points PEC estimates varied weakly with the time of a day and reached the value of several TECU for the condition of solar minimum. Percentage contribution of PEC to GPS TEC indicated the clear dependence from the time with maximal values (more than 50–60%) during night-time and lesser values (25–45%) during day-time.     

3D Imaging of the OH mesospheric emissive layer

A new and original stereo imaging method is introduced to measure the altitude of the OH nightglow layer and provide a 3D perspective map of the altitude of the layer centroid. Near-IR photographs of the OH layer are taken at two sites separated by a 645 km distance. Each photograph is processed in order to provide a satellite view of the layer. When superposed, the two views present a common diamond-shaped area. Pairs of matched points that correspond to a physical emissive point in the common area are identified in calculating a normalized cross-correlation coefficient (NCC). This method is suitable for obtaining 3D representations in the case of low-contrast objects. An observational campaign was conducted in July 2006 in Peru. The images were taken simultaneously at Cerro Cosmos (12°09′08.2″ S, 75°33′49.3″ W, altitude 4630 m) close to Huancayo and Cerro Verde Tellolo (16°33′17.6″ S, 71°39′59.4″ W, altitude 2272 m) close to Arequipa. 3D maps of the layer surface were retrieved and compared with pseudo-relief intensity maps of the same region. The mean altitude of the emission barycenter is located at 86.3 km on July 26. Comparable relief wavy features appear in the 3D and intensity maps. It is shown that the vertical amplitude of the wave system varies as exp (Δz/2H) within the altitude range Δz = 83.5–88.0 km, H being the scale height. The oscillatory kinetic energy at the altitude of the OH layer is comprised between 3 × 10⁻⁴ and 5.4 × 10⁻⁴ J/m³, which is 2–3 times smaller than the values derived from partial radio wave at 52°N latitude.     

二维系统一般模型的正实控制

本文研究的是二维系统一般模型的正实控制。本文的目的是针对该模型,设计一个状态反馈控制器,使得闭环系统是稳定的并且闭环传递函数是延展严格正实的,所得到的解是通过线性矩阵不等式给出,通过解决该线性矩阵不等式可获得期待的状态反馈控制器。最后,我们提供了一个数值算例来验证提到方法的有效性。     

多体全自由飞过程的数值模拟

以三维非结构粘性直角网格重构为构架,数值求解了固定空间网格瞬间运动边界的N-S方程,逼近了流场的非定常过程,结合六自由度的弹道方程,对单体或多体运动过程进行了全自由飞数值模拟,数值模拟结果和级间分离的风洞自由飞试验进行了对比,初步的计算结果说明,全自由飞数值模拟在一定程度上可以描述风洞试验的飞行轨迹,并且适应能力更强,整个全自由飞数值模拟系统可以为更复杂的单体机动飞行或多体运动过程提供快速实用的数值模拟方法.     

双满壳层附近原子核的双粒子能谱

采用由M-3Y力等效G矩阵,用格林函数方法对Ca42、Sc42、N i58和Cu58的双粒子能谱做了理论计算和讨论.结果表明:二级图中3p1h不可约顶角考虑多重散射后,使能级更趋于实验能级.因此用格林函数方法计算双粒子能谱是十分有效的。