一组新的绳系卫星系统广义坐标

应用一组新的六维广义坐标,在一个统一的力学系统中,研究在外摄动力（地球非球形引力与大气阻力等）及系绳拉力的作用下,绳系系统质心在惯性空间的轨道运动,以及该系统相对于质心的相对运动。系绳模拟为具有质量的弹性连续体,系绳两端的空间飞行器假设为点质量。下列变量取为力学系统的广义坐标：系统质心的向径、赤经、赤纬,主星与子星之间的距离,以及系绳相对于系统质心子午面的两个欧拉角。经典的质心轨道根数,以及系绳在质心轨道面内与轨道面外的摆动角,均可由上述六个广义坐标及其广义速度确定。     

Possible Suzaku detection of non-thermal X-ray signals from a rotating magnetized white dwarf

Although rotating neutron stars (NSs) have been regarded as being textbook examples of astrophysical particle acceleration sites for decades, details of the acceleration mechanism remain a mystery; for example, we cannot yet observationally distinguish “polar cap” models from “outer gap” models. To solve the model degeneracy, it is useful to study similar systems with much different physical parameters. Strongly magnetized white dwarfs (WDs) are ideal for this purpose, because they have essentially the same system geometry as NSs, but differ largely from NSs in the system parameters, including the size, magnetic field, and the rotation velocity, with the induced electric field expected to reach 10¹³–10¹⁴ eV. Based on this idea, the best candidate among WDs, AE Aquarii, was observed with the fifth Japaneses X-ray satellite, Suzaku. The hard X-ray detector (HXD) on-board Suzaku has the highest sensitivity in the hard X-ray band over 10 keV. A marginal detection in the hard X-ray band was achieved with the HXD, and was separated from the thermal emission. The flux corresponds to about 0.02% of its spin-down energy. If the signal is real, this observation must be a first case of the detection of non-thermal emission from WDs.     

Monte Carlo calibration of the response of the University of Chicago’s Cosmic Ray Nuclei Experiment (CRNE) on IMP-8 to electrons above 0.5 MeV

Modern instrument-simulation techniques offer the possibility of increasing the scientific yield from archival space datasets. In this paper, we report on a simulation of the electron response of the University of Chicago’s Cosmic Ray Nuclei Experiment (CRNE) instrument on the IMP-8 satellite. IMP-8/CRNE returned data from 1973 to 2006. The CRNE particle telescope was designed to measure the isotopic composition of Galactic cosmic-ray (GCR) nuclei and has also been used in many studies of protons and ions above 10 MeV/nucleon from solar energetic particle (SEP) events. But CRNE also functions as a highly-capable detector for solar electrons above 0.5 MeV, an energy range that has not been extensively studied. Utilization of the CRNE electron data has heretofore been limited by the fact that CRNE was never calibrated for electrons. We have therefore used the GEANT4 Monte Carlo simulation package to model the CRNE response to electrons and (separately) protons for multiple energies and incident angles. The results were used to compute the energy- and angle-dependence of the effective area and the energy-dependence of the geometric factor. The response to protons, which was already well understood, was used to verify the mass model, the simulation settings, and the post-processing software. Our simulation of the IMP-8/CRNE electron response now allows analysis of hundreds of relativistic solar electron events observed by CRNE over the years, including studies of evolution of electron energy spectra with high time resolution. We show examples of these results and briefly discuss potential applications to future scientific investigations.     

Object injection in geodesic conditions: In-flight and on-ground testing issues

In absence of forces, any object moves along the straightest possible path in space–time, called geodesic. The presence of a gravity field generates a space–time distortion that reflects on a curvature of the geodesics. Outer space yields a privileged environment to achieve high levels of geodesic purity, thanks to the absence of many non-gravitational force disturbances typical of the Earth, mainly due to the atmosphere, micro-seismic activity, stray electro-magnetic fields, etc. Many experiments in the field of Fundamental Physics, General Relativity and Earth Observation are performed through space missions, in which objects are either set in geodesic conditions or their deviation from a geodesic is measured. In both cases, stray non-gravitational forces acting on them must be reduced to a negligible level.     

Correlation between the cosmic noise absorption calculated from the SARINET data and the energetic particles measured by MEPED: Simultaneous observations over SAMA region

The cosmic noise absorption is presented in terms of two-dimensional images obtained from the imaging riometers operated at the Southern Space Observatory (geographic coordinate: 29.4° S, 53.1° W), in São Martinho da Serra, Brazil, Concepcion (geographic coordinate: 36.5° S, 73.0° W) and Punta Arenas (geographic coordinate: 53.0° S, 70.5° W) in Chile, which belong to the South American Riometer Network and are located at the central and periphery regions of the South American Magnetic Anomaly. Correlations are performed between the maximum cosmic noise absorption observed at these stations and the energetic electron flux in two energy channels (>30 and >300 keV) and the proton flux in three energy channels (80–240, 800–2500 and >6900 keV) as measured by the Medium Energy Proton and Electron Detector, during a moderate geomagnetic storm that occurred on September 3, 2008. The results show high correlations between the cosmic noise absorption detected at São Martinho da Serra and the flux of protons with energy between 80 and 240 keV, and the flux of electrons with energies higher than 300 keV, while an additional ionization at Concepcion was correlated with electrons of energies higher than 30 keV. The cosmic noise absorption detected at Punta Arenas was probably caused by the increase of the protons flux with energy between 80 and 240 keV.     

用于飞机零部件制造装配的柔性工装数控系统(英文)

研究了柔性工装计算机数字控制(Computer numerical control,CNC)系统,该系统适于控制多种用于飞机零部件制造和装配的柔性工装设备。给出了柔性工装的机械结构分类,分析了柔性工装设备的控制需求。同时提出了一种CNC系统的硬件和软件架构,并予以实现。该系统利用配置参数描述柔性工装的机械结构。根据配置参数,CNC系统可以自动生成其控制功能和人机界面(Human machine interface,HMI)操作功能。将该CNC系统应用于某蒙皮-桁条装配柔性工装设备,结果证明了系统的有效性。     

基于创收的高职院校财务管理研究

随着高职教育的发展,创收已突破高职教育服务区域经济和社会发展的瓶颈成为当务之急,但目前高职院校在大力开展创收过程中存在着观念落后、财务分析不够、分配不尽合理等诸多财务管理方面的问题。加强对创收项目的财务管理,充分发挥创收的经济效益,必须更新管理观念,增强服务意识;必须规范会计核算,加强财务分析;明晰财务关系,合理分配收入。     

乔治·斯坦纳阐释学翻译理论观照下的译者主体性——以《聊斋志异》两个英译本的对比分析为例

以英国著名翻译理论家乔治·斯坦纳基于阐释学的翻译四步骤理论为指导,以《聊斋志异》两个英译本为研究对象,分析翻译活动中不同译者发挥其主体性造成的翻译差异,以研究译者主体性在翻译活动中的体现.     

纳米CuO/AP复合粒子的制备及催化性能研究

采用溶剂-非溶剂法制备出了以纳米CuO为核、AP为壳的CuO／AP复合粒子。TEM、KRD及从的测试结果表明。复合粒子中只有CuO和AP存在,且AP包覆于CuO的外表,而DSC对复合粒子催化性能的测试结果表明。纳米CuO／AP复合粒子中AP的高温分解峰温度下降到101℃,较CuO-AP的简单混合物提前了5．64℃,而且复合粒子中AP的低温分解峰消失,在完成由斜方晶系向立方晶系的晶型转变后,便直接进入了高温分解,这为改善推进剂燃速提供了一条可行途径。     

硼粒子直径对点火位置及燃烧效率的影响研究

采用颗粒轨道模型对非壅塞固冲发动机补燃室内不同直径硼粒子的点火及燃烧进行了数值模拟。其中,气相反应简化为一种等效气体的燃烧,硼粒子与O2的燃烧反应模型采用涡耗散模型。硼粒子的点火过程采用King模型,燃烧过程采用化学动力学控制的燃烧模型。结果表明,直径较小的硼粒子能够在补燃室头部点火,且能随气流旋转,驻留时间较长,燃烧较为充分,直径较大的硼粒子与此相反。