有质量喷注和边界移动圆柱形流管中的声稳定性

本文利用Ｖａｎ Ｍｏｏｒｈｅｎ提出的平均处理法，从理论上分析了一维流管通道随时间变化和燃烧边界运动对燃烧室线性声稳定性的作用。得出结论是，空腔的瞬态扩大和边界运动平衡掉了一部分声能。     

The Pre-CME Sun

The coronal mass ejection (CME) phenomenon occurs in closed magnetic field regions on the Sun such as active regions, filament regions, transequatorial interconnection regions, and complexes involving a combination of these. This chapter describes the current knowledge on these closed field structures and how they lead to CMEs. After describing the specific magnetic structures observed in the CME source region, we compare the substructures of CMEs to what is observed before eruption. Evolution of the closed magnetic structures in response to various photospheric motions over different time scales (convection, differential rotation, meridional circulation) somehow leads to the eruption. We describe this pre-eruption evolution and attempt to link them to the observed features of CMEs. Small-scale energetic signatures in the form of electron acceleration (signified by nonthermal radio bursts at metric wavelengths) and plasma heating (observed as compact soft X-ray brightening) may be indicative of impending CMEs. We survey these pre-eruptive energy releases using observations taken before and during the eruption of several CMEs. Finally, we discuss how the observations can be converted into useful inputs to numerical models that can describe the CME initiation.     

开关寿命连续型不可修冷、温贮备系统的可靠性分析及其随机模拟

本文对由n个部件组成的、开关寿命为连续型随机变量的不可修冷、温贮备系统作了可靠性分析,建立了这两类系统的一般模型,给出了冷贮备系统可靠度R_n(t)及平均寿命MTTF的一般形式解。并在指数分布场合下,给出了R_n(t)及MTTF的解析表达式。当部件贮备寿命相互独立同分布时,温贮备系统可以通过一个虚设的开关变量而归结为冷贮备系统。对一般的贮备系统,可以运用数理统计方法,根据样本给出R_n(t)及MTTF的估计。文末利用随机模拟方法,构造所需样本,便可获得R_n(t)及MTTF的数值估计。实例表明,随机模拟的结果是令人满意的。     

超长大直径钻孔灌注桩桩端承载力研究

阐述了超长大直径钻孔灌注桩桩端承载力的影响因素,包括施工工艺、深度效应和尺寸效应等。分析和对比了目前国内常用的各规范所采用的计算方法。文中算例的计算结果表明,对于同等条件的桩,各规范的计算结果相差较大。采用自平衡试桩法获得了几个重大工程的超长大直径钻孔灌注桩的桩端承载力的实测值。将工程实例的测试结果与各规范的计算结果进行对比,证实了目前规范的计算方法不尽合理。目前各规范中桩端承载力的计算方法是在针对小直径的中短桩的研究基础上建立的。如今,大型桥梁工程中普遍采用超长大直径钻孔灌注桩的情况下,对其桩端承载力的计算应当进行相应的调整,使设计更为合理。     

带翼梢外挂的CK1机翼颤振分析

本文根据颤振运动方程,应用v～g参数法和非定常气动力的偶极子格网法计算了CK1机翼翼尖带外挂物红外器时的颤振,分析了翼尖外挂物对机翼颤振的影响,确定翼尖外挂有利的配置方案.计算结果表明CK1机翼的颤振对梢部的重量分布是敏感的,红外器的弦向位置及翼尖配重布置得当,则可提高颤振速度,否则也可降低颤振速度。     

激波过弯道绕双圆柱流场

采用单曝光光栅干涉或双曝光光栅干涉，研究激波过弯道绕双圆柱传播的微波流场。采用单曝光法，成功显示入射激波到第一圆柱上的反射、绕射，到达第二圆柱上的反射、绕射。在同一底片上采用双次曝光，第一次脉冲记录直道上的平面波，第二次脉冲记录激渡过弯道绕双圆柱流场。这些照片对于研究反射、绕射及它们边界的相互作用是很有用的。     

彩色三维激光快速成型技术的研究

目前逆向工程采用线结构激光和一个彩色面阵CCD摄像机构成三维彩色扫描系统,彩色CCD摄像机分两次对被测物体成像,首先摄取物体的彩色图片,然后加用滤光片再摄取激光光平面上的三维信息.最后将两次获取的信息重叠,便可得到三维彩色信息.提出了激光光平面方程式三维测量方法,建立了相应的数学模型.研制成一套适用于彩色逆向工程流程,并进行了实验研究,给出了实验结果.     

Biological life support for manned missions by ESA.

The anticipated evolution of life support technologies for ESA, considering both the complementary life support system requirements and the missions' characteristics, is presented. Based on these results, promising biological life support technologies for manned space missions have been selected by ESA either for their intrinsic ability and performance in effecting specific tasks for atmosphere-, water-, waste-management versus physico-chemical alternatives and/or for longer-term application to a more ecological concept (CES) focusing ultimately on food production. Actual status and plan for terrestrial and space testing of biological life support presented focusing on the "task specific" decontamination technology of the Biological Air Filter (BAF), and on food reprocessing technologies from biodegradable wastes with the MELISSA microbial ecosystem.     

Observation of fundamental magnetoplasma emissions excited in magnetosphere by modulated electron beams

There were several cases when modulated electron beam had been injected from APEX satellite into an otherwise unmodified ionospheric plasma. The beams were formed from 2 μs pulses repeated at a rate of 40kHz. Injections took place in the altitude range 400–1100km over Europe. The onboard receiver connected to the dipole antenna swept the frequency interval 1–10 MHz in 1 sec. Due to a relatively narrow receiver bandwidth (15 kHz), moderate frequency step (50 kHz), slow changes of f_n and f_c (local electron plasma and gyro frequencies) fine structure of excited emissions was detected. In many cases, a very prominent doublet could be convincingly identified as a (f_n,f_u=sqrt(f_n^*f_n+f_c^*f_c)) band, with f_n practically equal to the local plasma frequency in the unperturbed ionosphere. Determination of plasma frequency is of prime importance in analysis of complex structures composed from various harmonics f_n,f_c,f_u. Complexity is manifested as coalescing of various harmonics with maxima shifted from nominal frequencies or splitting them into components due to mixing of local and propagation effects. Despite the existence of strong emissions on frequencies characteristic for the unperturbed ionosphere, very strong broadcasting transmissions are frequently cut off, even when the beam is directed upward. Most typical spectra are discussed.