具有确定弧数最长路的算法

给出了寻求强连通赋权有向图中从一顶点到任意顶点间具有确定弧数的最长路 (最短路 )和最长初等路 (最短初等路 )的算法 ,并对算法的有效性进行了讨论。该算法对扩展 Karp和Cohen的结果——强连通赋权图中最小平均权的算法和线性离散事件系统的闭环系统矩阵在极大代数意义下的特征值的算法 ,具有实际意义     

涡轮叶片的循环蠕变分析

研究了航空发动机一级涡轮叶片的蠕变行为。对叶片的危险区作了静载恒温蠕变计算和变温变载蠕变计算。其结果是静载恒温蠕变和实验结果一致;其循环蠕变变形略小于静蠕变变形。变温变载下叶片的蠕变寿命可用静载恒温蠕变进行预估。      

热循环对某热控涂层热辐射的影响

对某热控涂层进行了快速高低温循环试验(-196~900℃),通过太阳吸收比、半球发射率检测和SEM形貌等对涂层的热辐射性能进行分析。实验表明,经过热循环后,该涂层保持高吸收比的稳定状态(0.87左右),而半球发射率从原始的0.57提高到0.72,最后稳定在0.75左右。SEM微观形貌研究表明,热循环实验使涂层表面的结晶度和晶粒大小发生变化,导致涂层热辐射性能改变。     

20kHz下TC17钛合金超高周疲劳性能研究

应用基于压电超声疲劳试验技术开发的20kHz弯曲疲劳试验系统,完成了室温下TC17合金超高周疲劳试验.结果表明:在疲劳循环大于107周次时,试样仍会发生疲劳断裂,疲劳强度随循环次数的增加而下降,并不存在明显的疲劳极限.TC17合金的应力-寿命(S-N)曲线在107~109周次的范围内为连续下降型.光学显微镜发现,TC17合金的疲劳破坏主要起源于试样表面.当存在夹杂物时,疲劳裂纹从距离表面很近的夹杂物处萌生,能谱分析表明夹杂物的成分主要是铝的氧化物.      

某机翼的安全预测载荷模型建立

基于试飞阶段全V-N包线的实测飞行载荷，将改进遗传算法、线性回归与BP神经网络融合，给出了一种适用于全寿命周期的自适应安全预测载荷模型建立方法。将该方法应用于某飞机机翼的安全预测载荷模型建立，并对所建立的载荷模型进行了全V-N包线的验证。分析了样本空间与载荷模型精度的关系。结果表明：建立的弯矩预测载荷全包线最大误差为10.6%、平均误差为1.0%，剪力的最大误差为9.1%、平均误差为0.4%，比优化线性和分段线性的误差小，比神经网络的收敛性好。随着建模数据从全样本、1/2、1/3、…、1/10样本的变化，弯矩和剪力方程的全V-N包线的最大误差整体呈增大趋势，弯矩最大误差变化范围为10.6%~19.6%，最大剪力误差变化范围为9.1%~27.9%。     

Limit cycles of accretion disks in the Rapid Burster and GRS 1915+105

The Rapid Burster is known to show rapidly repetitive bursts (Type II bursts). An interesting feature of the Type II burst is an approximate proportionality of the burst duration to the time to the next burst. The time sequence from a burst to the following quiescent phase can be said to be a time-scale invariant high (burst phase)–low (quiescent phase) transition. The Galactic superluminal source, GRS 1915+105 exhibits a variety of the time variation of the X-ray flux and often repeats transitions between a high-flux level and a low-flux level. In such high–low transitions, Belloni et al. (1997b) found an approximate proportionality between the duration of the low-flux phase and that of the following high-flux phase, over a wide range of the time scale. This low–high transition can again be said to be time-scale invariant. However, an interesting difference between the two time scale invariant transitions is an opposite order of the high and low-flux phase in the time-scale invariant sequence. In the case of the Rapid Burster, the high-flux (burst) phase is the first, while the low-flux phase is the first in the case of GRS1915+105. A limit cycle between an accretion disk in a state of the standard-disk and that in a state of the ADAF (advection dominated accretion flow) is discussed to explain the time-scale invariant high–low (or low–high) transition as well as the difference between the neutron star system and the black-hole system, qualitatively. A phenomenological relation of the accretion disk change with mass ejections from the central part of the disk is also discussed.     

航空发动机关键件循环寿命耗损实时监视软件设计

介绍了航空发动机循环寿命耗损实时监视软件设计的原理和结构框架,重点介绍了历程数据实时处理方法,经实用表明,该软件操作简单,能够准确监视发动机部件的耗损循环数,具有一定的军事和经济价值。     

Solar ring mission: Building a panorama of the Sun and inner-heliosphere

Solar Ring (SOR) is a proposed space science mission to monitor and study the Sun and inner heliosphere from a full 360° perspective in the ecliptic plane. It will deploy-three 120°-separated spacecraft on the 1-AU orbit. The first spacecraft, S1, locates 30° upstream of the Earth, the second, S2, 90° downstream, and the third, S3, completes the configuration. This design with necessary science instruments, e.g., the Doppler-velocity and vector magnetic field imager, wide-angle coronagraph, and in-situ instruments, will allow us to establish many unprecedented capabilities: (1) provide simultaneous Doppler-velocity observations of the whole solar surface to understand the deep interior, (2) provide vector magnetograms of the whole photosphere — the inner boundary of the solar atmosphere and heliosphere, (3) provide the information of the whole lifetime evolution of solar featured structures, and (4) provide the whole view of solar transients and space weather in the inner heliosphere. With these capabilities, Solar Ring mission aims to address outstanding questions about the origin of solar cycle, the origin of solar eruptions and the origin of extreme space weather events. The successful accomplishment of the mission will construct a panorama of the Sun and inner-heliosphere, and therefore advance our understanding of the star and the space environment that holds our life.