提高企业经济效益的模块化技术

介绍了模块化技术 ,并从不同角度分析了模块化技术是提高企业经济效益的有效途径。     

Thermal cyclotron radiation from a hot coronal loop with helical magnetic field

The spectral and polarization properties of thermal cyclotron radio emission from a hot coronal loop with a current along the axis are computed. The magnetic field is supposed to have a component along the loop axis as well as a poloidal part due to the current, both components being of comparable magnitude. In this specific configuration a helical magnetic field is present with a remarkable minimum of its absolute value along the loop axis and a maximum at its periphery. The presence of one or two maxima of magnetic field value along the line of sight results in increasing optical thickness of the gyroresonance layers at appropriate frequencies in the microwave band and, therefore, in enhanced radio emission at those harmonics which are optically thin (for example,s=4). These cannot be observed in models with the commonly employed magnetic field configuration (longitudinal along the loop axis).We show that the frequency spectrum of thermal cyclotron radiation from a hot coronal loop with a helical magnetic field differs from that of the standards-component source (with smooth frequency characteristics and polarization corresponding toe-mode) in that plenty of fine structures (line-like features and cut-offs) are present and theo-mode is prevalent in some frequency intervals. The enhanced radio emission at high harmonics and the complicated form of frequency spectrum in the model considered imply that some microwave sources, which are poorly explained in traditional models of solar active regions, may be associated with helical magnetic fields in hot coronal loops. Computations allow one to indicate spectral and polarizational peculiarities of local sources testifying to the presence of a helical magnetic field.     

国内外航天器密封舱主结构材料的选用

介绍了国内外航天器密封舱主结构常用的铝合金材料,并对其常规力学性能、断裂韧度、焊接性能、抗应力腐蚀性能等进行了比较。同时,结合不同的使用环境及条件对可选材料进行了分析,给出了目前及未来密封舱主结构材料的选择建议。文章研究结果可为大型航天器密封舱主结构研制提供参考。     

用户星中继终端在轨应用策略

在介绍在轨用户星中继终端的分类、功能和使用现状的基础上,重点对用户星中继终端多约束条件进行了梳理分析。为缓解常态化应急测控带来的资源紧张矛盾,提出了用户星中继终端在轨应用策略,即Ka/S模式下影随测控,小S模式下定时捕获。针对Ka+小S模式下实现影随测控的可行性问题,利用STK(Satellite Tool Kit,卫星开发工具包)软件进行了仿真计算分析,结果表明:为实现影随测控,满足测控快速响应需要,要求星载S频段中继测控天线对中继卫星的覆盖范围,应大于星载中继数传天线对中继卫星的覆盖范围。     

氦气驱动预压涡轮泵启动初期反流问题分析

用于某液体火箭发动启动动系统的气驱预压涡轮泵在起动初期出现了气体反流,导致预压泵呈夹气状态,对发动启动动过程控制不利。根据驱动试验系统原理,在MWorks平台中对驱动过程进行了仿真。对预压泵采用了Suter全特性表达式,对涡轮管路及排放路分别建立了描述排空与两相流动过程的简化数学模型。结果 表明,导致反流的原因为涡轮入...     

石英晶振微天平湿度传感器响应特性研究

石英晶振微天平传感器是传感器研究的一个热点,文中介绍了自行研制的一种以SPPESK为敏感元件的石英晶振湿度传感器,利用差频法测量了传感器的静态稳定性、重复性和线性度、灵敏度和动态响应。结果表明: 该传感器具有良好的定动态响应特性,能够用于实际气体湿度的检测。     

大芯径大数值孔径光纤测试系统测量不确定度评定

简述了大芯径大数值孔径光纤测试系统的测量原理，建立了测试系统的数学模型并对该系统的测量不确定度进行了评定。     

Comparative analysis of chemical composition and optical properties of gaseous and disperse phases of the Earth-group planetary atmospheres

The models of chemical composition and structure of the Earth-type planetary atmospheres are offered. The optical properties of gaseous and disperse phases of the atmospheres are investigated.     

Wave measurements in active experiments on plasma beam injection

The paper presents the results and discussion of VLF wave measurements carried out in the course of two rocket experiments on injection of a dense cesium ion beam into the ionosphere at the heights of 165–240 km. The injection was accompanied by enhancement of the broad-band noise by several orders of magnitude. The wave measurements in the frequency range of 1–11 kHz revealed two pronounced frequencies somewhat exceeding that of the lower-hybrid resonance oscillations in the background plasma and the cesium beam. The oscillations were modulated by frequencies close to the ion-cyclotron frequencies of the background plasma.     

Preliminary data of the thermal regime and circulation in the upper mesosphere and mesopause

Circulation and thermal structure for the 90–95 km region is described on the basis of the joint analysis of direct and indirect sounding data. Mean season charts of the 0.001 mb surface were compiled using data from meteor trials, ionospheric drifts, rocket launchings and data of the rotational temperature of hydroxyl emission.