Orbital phase spectroscopy of X-ray pulsars to study the stellar wind of the companion

High Mass X-ray Binary Pulsars (HMXBP), in which the companion star is a source of supersonic stellar wind, provide a laboratory to probe the velocity and density profile of such winds. Here, we have measured the variation of the absorption column density along with other spectral parameters over the binary orbit for two HMXBP in elliptical orbits, as observed with the Rossi X-ray Timing Explorer (RXTE) and the BeppoSAX satellites. A spherically symmetric wind profile was used as a model to compare the observed column density variations. In 4U 1538-52, we find the model corroborating the observations; whereas in GX 301-2, the stellar wind appears to be very clumpy and a smooth symmetric wind model seems to be inadequate in explaining the variation in column density.     

PC—DIO─96接口板在大尺寸计量标准中的应用

介绍了美国NI公司的数据采集板PC—DIO—96的功能,及其在Windows95下软硬件的安装,描述了如何使用其随板软件包,并给出了其三种主要功能（线功能、口功能和组功能）的程序框图。详细介绍了在“建立大尺寸计量标准”题目中应用该板进行环境参数的采集和电机控制。     

CBERS-1卫星IRMSS数据及融合技术在鸭绿江口示范应用评价

文章通过丹东鸭绿江口与大连地区典型研究中采用的 CBERS-1卫星IRMSS数据,对数据图像的质量、图像信息的处理方法和专业应用潜力进行评价。通过评价IRMSS不同波段数据的应用效果,加速IRMSS数据的推广应用。     

微重力火箭设计中减旋方案等问题

讨论了一种微重力火箭总体设计中减旋方案，飞行载荷，气动加热与壁温计算等几个关键问题。结合该火箭的具体特点，提出了一种简单实用的被动式减旋措施，即，安装反旋尾翼及辅助减旋机构，并分析了减旋与动稳定性的关系。对超高音速火箭的飞行载荷和气动热进行了分析计算。     

回收着陆半实物仿真系统程控装置模拟程序设计

文章描述了回收着陆半实物仿真系统的整个框架，针对整个半实物仿真系统的设计需要和回收程控装置的特点，设计了回收程控装置模拟程序。在程序中所选择的定时方法既满足实时仿真的需要，保证了定时的精度又提高了程序的效率。该程序和半实物仿真系统为回收程控装置设计人员提供了一个快捷的平台来修改程控装置的设计时序。     

天基空间目标监视可见光遥感器研究

文章通过对美国天基可见光遥感器SBV性能和关键技术的分析，提出了发展中国天基空间目标监视可见光遥感器的建议。     

模糊控制在导弹瞬态气动热流试验中的研究

导弹与高速飞行器气动模拟试验瞬态热控过程的特点是变化复杂、瞬变、高度非线性、强耦合,很难或者根本无法建立控制的数学模型.模糊控制具有鲁棒性好,对参数变化的适应性强,过渡过程时间短等常规控制方法所不能比拟的优点.将模糊控制方法应用于导弹瞬态气动加热模拟控制系统,使该系统能够按照导弹高速飞行过程中弹体表面热流的瞬态连续变化对气动模拟加热过程实施快速的动态控制.     

变螺距螺纹加工的参数化编程

文章阐述了变螺距螺纹加工的编程方法,探讨了用宏程序实现变螺距螺纹的参数化编程,提高了编程效率,增强了程序的灵活性和通用性。     

Evolution of the temporal and the spectral properties in 2010 and 2011 outbursts of H 1743-322

The Galactic black hole candidate H 1743-322 exhibited two X-ray outbursts in rapid succession: one in August 2010 and the other in April 2011. We analyze archival data of this object from the PCA instrument on board RXTE (2–25 keV energy band) to study the evolution of its temporal and spectral characteristics during both the outbursts, and hence to understand the behavioral change of the accretion flow dynamics associated with the evolution of the various X-ray features. We study the evolution of QPO frequencies during the rising and the declining phases of both the outbursts. We successfully fit the variation of QPO frequency using the Propagating Oscillatory Shock (POS) model in each of the outbursts and obtain the accretion flow parameters such as the instantaneous shock locations, the shock velocity and the shock strength. Based on the degree of importance of the thermal (disk black body) and the non-thermal (power-law) components of the spectral fit and properties of the QPO (if present), the entire profiles of the 2010 and 2011 outbursts are subdivided into four different spectral states: hard, hard-intermediate, soft-intermediate and soft. We attempt to explain the nature of the outburst profile (i.e., hardness-intensity diagram) with two different types of mass accretion flow.     

流体力学综合实验台的开发与应用

以创新型、综合型实验设计为目标,通过对流体力学综合实验台功能的设计与开发,突出其综合应用性和对实践教学效果的促进作用;对实验数据进行分析,说明实验台设计的合理性。