发动机安装损失试验精确测温方法研究

直升机发动机装机后,一般都需进行安装损失的飞行试验,通过发动机进气温升与进气压损等数据的测量,利用发动机性能计算软件,分析装机状态下的发动机性能变化。UMA2000数据采集系统预设的蕈程相对于发动机温升的变化范围过宽,往往导致较大的测量误差,直接影响发动机安装损失的分析结论。通过在UMA2000数据采集系统引入偏置电压的方法,实现了发动机进气温升测量精度的大幅提高。     

微波虚拟时频分析仪的分析与设计

指出了经典的时域分析法与频域分析法存在的主要问题 ,然后在虚拟示波器和虚拟频谱分析仪的基础上提出一种微波虚拟时频分析仪的设计方案。简述了此虚拟仪器的功能 ,重点阐述了在仪器开发过程中软硬件的设计 ,并探讨了设计的关键技术及难点     

Equilibration Processes in the Warm-Hot Intergalactic Medium

The Warm-Hot Intergalactic Medium (WHIM) is thought to contribute about 40–50% to the baryonic budget at the present evolution stage of the universe. The observed large scale structure is likely to be due to gravitational growth of density fluctuations in the post-inflation era. The evolving cosmic web is governed by non-linear gravitational growth of the initially weak density fluctuations in the dark energy dominated cosmology. Non-linear structure formation, accretion and merging processes, star forming and AGN activity produce gas shocks in the WHIM. Shock waves are converting a fraction of the gravitation power to thermal and non-thermal emission of baryonic/leptonic matter. They provide the most likely way to power the luminous matter in the WHIM. The plasma shocks in the WHIM are expected to be collisionless. Collisionless shocks produce a highly non-equilibrium state with anisotropic temperatures and a large differences in ion and electron temperatures. We discuss the ion and electron heating by the collisionless shocks and then review the plasma processes responsible for the Coulomb equilibration and collisional ionisation equilibrium of oxygen ions in the WHIM. MHD-turbulence produced by the strong collisionless shocks could provide a sizeable non-thermal contribution to the observed Doppler parameter of the UV line spectra of the WHIM.     

Thermodynamical Properties of the ICM from Hydrodynamical Simulations

Modern hydrodynamical simulations offer nowadays a powerful means to trace the evolution of the X-ray properties of the intra-cluster medium (ICM) during the cosmological history of the hierarchical build up of galaxy clusters. In this paper we review the current status of these simulations and how their predictions fare in reproducing the most recent X-ray observations of clusters. After briefly discussing the shortcomings of the self-similar model, based on assuming that gravity only drives the evolution of the ICM, we discuss how the processes of gas cooling and non-gravitational heating are expected to bring model predictions into better agreement with observational data. We then present results from the hydrodynamical simulations, performed by different groups, and how they compare with observational data. As terms of comparison, we use X-ray scaling relations between mass, luminosity, temperature and pressure, as well as the profiles of temperature and entropy. The results of this comparison can be summarised as follows: (a) simulations, which include gas cooling, star formation and supernova feedback, are generally successful in reproducing the X-ray properties of the ICM outside the core regions; (b) simulations generally fail in reproducing the observed “cool core” structure, in that they have serious difficulties in regulating overcooling, thereby producing steep negative central temperature profiles. This discrepancy calls for the need of introducing other physical processes, such as energy feedback from active galactic nuclei, which should compensate the radiative losses of the gas with high density, low entropy and short cooling time, which is observed to reside in the innermost regions of galaxy clusters.     

Kuafu and the studies of CME initiation

We first briefly review the current trend in the studies of coronal mass ejections (CMEs), then summarize some recent efforts in understanding the CME initiation. Emphasis has been put on the studies of Earth-directed CMEs whose associated surface activity and large scale magnetic source have been well identified. The data analysis by combining the MDI full disc magnetograms, vector magnetograms of active regions, EUV waves and dimmings, non-thermal radio sources, and the SOHO LASCO observations has shed new light in understanding the CME magnetism. However, the current studies seem to invoke new observations in a few aspects: (1) The observations which enable us to trace CMEs from the earliest associated surface activity to its initial acceleration and key development in the low corona in the height of 1–3 R; (2) The imaging spectroscopic observations which can be used to diagnose the early plasma outflow and the line-of-sight velocity in understanding the kinematics of CMEs; (3) The accurate timing from primary magnetic energy release, manifested by chromospheric activity, non-thermal radio bursts, and EUV, X-ray and γ-ray emissions, to the CME initiation, early acceleration and propagation, and the consequences in the interplanetary space and magnetosphere. The Kuafu Mission will meet the basic requirement for the new observations in CME initiation studies and serve as a monitor of space weather of the Sun–Earth system.     

分布式卫星系统的协同导航估计方法

针对分布式卫星系统对合作目标的协同导航估计问题,提出了前端与后端结合的一种分布式协同导航方法。前端基于一致性算法对无迹卡尔曼滤波方法进行改造进而完成设计,后端基于协方差交集算法并利用快速权值计算方法以及非可加性参数融合方法进行设计。最后基于Matlab以及STK轨道传播模型进行了数值仿真,得到了预期的仿真结果,验证了方法的有效性。     

分包系统的星上数据源及其模型

分包体制的星载数据系统与传统的 PCM遥测遥控系统两者面向的数据源有很大不同。描述分包系统各种星上数据源 ,分析其特点后 ,提出了一种通用的建模方法 ,并通过举例说明。在系统设计、仿真和测试中 ,这种方法都是很有用的。     

Changes in the Structure of Comet Nuclei Due to Radioactive Heating

The initial structure of a comet nucleus is most probably a homogeneous, porous, fine-grained mixture of dust and ices, predominantly water. The water ice is presumably amorphous and includes considerable fractions of occluded gases. This structure undergoes significant changes during the early evolution of the nucleus at large heliocentric distances, due to internal radiogenic heating. Structural changes occur mainly as a result of gas flow through the porous medium: the gas pressure that builds up in the interior is capable of breaking the fragile structure and altering the pore sizes and porosity. These effects are modeled and followed numerically, testing a large number of parameters. This revised version was published online in June 2006 with corrections to the Cover Date.     

测量船多设备外测数据的融合算法

为了进一步提高航天测量船外弹道数据处理的精度,须根据不同的任务特点和要求选用合适的数据处理方法。针对测量船精度校飞时多设备同时跟踪飞行目标的工程背景,提出多设备外弹道数据融合处理的构思,根据数据融合的原理阐述了数据融合技术在精度校飞数据处理中的应用,给出目标位置融合的几种算法,并用加权最小二乘数据融合算法对实测数据进行处理。工程应用结果表明：本文提出的数据融合方法计算量少、精度高,适合工程应用。     

劳资管理系统的设计及实现

针对劳资管理的实际情况利用 Ｆｏｘｐｒｏ２ ．５ｂ 开发了劳资管理系统软件,该软件首次采用双数据库的设计思想来完成对劳资数据库进行显示、打印、统计等操作。使劳资管理工作的自动化程度得到了明显的提高。