基于电离层加热的人工沿场散射RCS估计

在电离层加热理论研究和试验研究的基础上, 根据F层散射体的特征和不均匀体散射理论, 建立了人工沿场散射(AFAS)中散射体的散射截面积数学模型. 通过与国际上理论结果对比, 证明了模型的适用性. 利用模型估算了中国人工沿场散射通信中, 通信频段在20~100 MHz时散射体的散射截面积, 结果显示, 甚高频率(VHF)的低端可达80 dB•m2. 另外, 通过计算验证了雷达波束垂直地磁场方向时可获得最大散射截面积的理论.      

INTERFACIAL MASS TRANSPORT IN OXIDE CRYSTAL GROWTH

A space high temperature in situobservation instrument (SHITISOI) is dedicated to visualize and record the whole growth process of oxide crystal in high temperature melts and solutions. Model experiments using transparent liquids such as KNbO3,Li2B4O7+KNbO3 were chosen to investigate effects of interracial mass transport in oxide crystal growth. For the scaling of the coupled velocity, heat and concentration fields in KNbO3 crystal growth, a rotating crystal growth process was performed and the widths of interfacial concentration, heat and momentum transition zones (The "boundary layers") are obtained, which are 7.5×10-a, 8.6×10-2 and 4.4×10-1 cm,respectively. Hence one can expect that interfacial concentration gradient will be confined to a narrow layer and in region of major concentration change at the in terface. In order to study a mechanism based on the interfacial mass transport resulting from hydrodynamics, the growth of KNbO3 grain in high temperature Li2B4O7 and KNbO3 solutin was studied. The result shows that the pivotal feature in the KNbO3 crystal growth is the initiated by KNbO3 solute surface tension gra dient which is caused by the slow diffusion of KNbO3 solutes. Direct comparison of the model predictions and experimental observed phenomena demonstrate the predictive capability of this model.     

Space Life Science of China

With the human space exploration activities, space life science is an emerging interdiscipline, which covers a wide range of researches. Based on our country's manned space station and recoverable satellite science experimental platform, the development of space life science research is very important to acquire new knowledge or new technological innovation, to give further services to the human space exploration activities, to improve the national economic and social development. Both ground-based and flight applied studies were continuously performed in the previous 2 years. Here, we review and summarize the researches on space life sciences contributed by Chinese scientists.      

EVALUATION OF MORPHOLOGY-STABLE CRITICAL SIZE OF KNbO3 CRYSTALS

Skeletal form of KNbO3 crystals growing in Li2B4O7 solvent was in-situ observed at 900°C and it was found that shallow depression started to develop on the surface of KNbO3 crystals when the crystal size exceeded several micron, typically 7 micron.Based on the quantitative criterion derived by Chernov, the estimated critical size of KNbO3 crystals was 1 micron, which was consistent with the experimental measure ment. The kinetic coefficients, kcorner and kcr, in the criterion were experimentally obtained in the diffusive-convective and diffusive-advective flow states respectively.     

Space Life Science of China in 2015

With the human space exploration activities, space life science is an emerging interdisciplinary and it covers a wide range of research. Based on our country's manned space station and recoverable satellite science experimental platform, the development of space life science research is very important to acquire new knowledge or new innovation in technology, to give further services to the human space exploration activities, to improve the national economic and social development. Based on present situation, both theoretical and applied researches were continuously performed in 2015. Here, we review and summarize the researches on space life sciences which were contributed by Chinese scientists.      

空间环境对InSb晶体生长的影响

为了研究太空微重力环境对InSb 晶体生长的影响,在空间进行了InSb 晶体的重熔和再结晶实验。实验结果表明,空间可以生长出结构较完整、组份均匀的高质量单晶。另外还证明了利用多用途单晶生长炉内一侧余热进行单晶生长的可行性。     

Science Researches of Chinese Manned Space Flight

With the complete success of the 2nd stage of Chinese Manned Space Program (CMSP), several science researches have been performed on Tiangong-1 experimental spacelab, which was docked with three Shenzhou spaceships one after another. The China's real spacelab, Tiangong-2 will be launched in 2015, docked with a Shenzhou spaceship soon. After six months, it will be docked with the first Chinese cargo ship (Tianzhou-1). More space science researches, involving with space biology, fluid physics, fundamental physics, materials science, Earth science, astronomy and space environmental science, will be operated on Tiangong-2 spacelab, and crewed and cargo spaceships. Furthermore, the considerable large-scale space utilization of Shina's Space Station is planned. The research fields include yet not limited to space medicine and physiology, space life science and biotechnology, fluid physics and combustion in microgravity, space material science, and fundamental physics in microgravity, space astronomy, Earth science, space physics and space environment utilization, technology demonstration.      

EFFECTS OF CONVECTIVE FLUID MOTION UPON OXIDE CRYSTAL GROWTH IN HIGH TEMPERATURE SOLUTION

For understanding of the influence of convective flow on crystal growth, space high temperature in situ observation instrument (SHITISOI) is dedicated to visualize and record the whole growth process of oxide crystals in high temperature up to 1000°C. Model experiments using transparent liquids such as KNbO3 and a mix ture of Li2B4O7+KNbO3 were chosen to investigate effects on ground and in space.On the earth, an investigation of growth kinetics of KNbO3 crystal related to two different states of convection: diffusive-advective flow and diffusive-convective flow,has been performed. The per unit length of a step e is calculated from the exper imental data for two different states of convection. Analyses of these data show the effect of buoyancy convection is to enhance the sharpness of the interface. The growth of KNbO3 crystals from solution of KNbO3+Li2B4O7 was investigated in space. The streamlines of the steady thermocapillary convection in Li2B4O7 solvent was observed. Due to thermocapillary convection, KNbO3 crystal grains grew and filled the whole solution homogeneously. Earth-based quenching experiments are de signed in order to study polyhedral instability of KNbO3 crystal, which is controlled by diffusion mechanism limitation. In all cases, when the crystal was nucleated near air/solution surface, it lost its polyhedral stability and varied from polyhedrons to dedrites. The thickness of diffusion mechanism limitation layer is about 60μm.     

Science Research of Microgravity Satellite SJ-10

The program SJ-10, one of the scientific satellite programs in the Strategic Priority Research Program on Space Science, the Chinese Academy of Sciences, was launched on April 6, 2016. There are totally 19 scientific payloads, a multi-function furnace for 8 material researches and three-dimensional cell cultures for the neural stem cell and the hematopoietic stem cell respectively. The recoverable satellite consists mainly of two capsules:a recoverable capsule was recovered on 18 April 2016, with all payloads of life science, the multi-function furnace and the payload for measurement of Soret Coefficients of Crude Oil (SCCO); and an un-recoverable capsule continued to work in additional 3 days with all other physics payloads. The experiments were operated via teleoperations, and all experimental data were received by the ground station in real time. The data and recoverable samples are analyzed by the experiment teams of the program.      

基于两种扫描方式的雷达探鸟系统

介绍了雷达探鸟系统的研究现状,包括以鸟击危害咨询系统为代表的大型雷达探鸟系统和以Accipiter为代表的机场雷达探鸟系统.基于X波段海事雷达搭建了"雷达探鸟实验系统",分别验证了其在水平和垂直两种扫描方式下探鸟的可行性.本系统在两种扫描方式下采集的两组探鸟雷达图像序列,分别由飞鸟目标提取算法进行处理.经过背景差分、噪声抑制、目标信息提取和数据融合,将鸟情信息从原始雷达图像中提取出来,并将其与卫星地图或高度坐标系相融合,融合图像直观地反映了探测区域内飞鸟目标的分布情况.最后,对国内外雷达探鸟系统的性能作了比较分析.     

在空间微重力下生长碲镉汞晶体

本文叙述了我国首次在空间微重力下进行的碲镉汞(MCT)晶体生长试验及一些观测结果。生长是从熔体进行的。在空间90min的加热时间内,将MCT多晶试样熔化,然后随炉冷却,最后在地面上再结晶。于是,生长出约3cm长的晶体,其表面光滑.结构致密,无孔洞,由1～3个大晶粒组成,其中单晶占74%。X射线能量色散分析(EDS)表明,其径向组分均匀性优于±0.02,其中约1cm长的一段晶体的径向组分均匀性优于±0.01。电学特性与地面上生长的样品基本相同。     

溶液法制备PVDF薄膜电活性相方法

为了制备具有电活性相的聚偏氟乙烯(PVDF)薄膜,采用了简单易操作的溶液涂膜方法,并研究了不同前驱体溶液浓度、搅拌时间以及热压工艺对PVDF不同电活性相的晶型结构形成的影响,利用X射线衍射仪、傅里叶变换红外光谱仪(FTIR)对PVDF薄膜的晶型结构进行分析.结果表明:前驱体溶液浓度7%~10%,搅拌时间2~3h都有利于β相的形成,利用红外光谱,可以计算β相的含量,在前驱体溶液浓度7%,搅拌时间2h时得到最大的β相含量81.3%;热压对PVDF薄膜的晶型结构有很大的影响,经过热压处理的PVDF薄膜中γ相转变成更加致密的β相.      

ADVANCES IN MATERIAL RESEARCHES UNDER MICROGRAVITY 2000-2002

The Engineering of Chinese Spacecraft provides Chinese scientists of materials great opportunity in the experiments for preparing materials under microgravity. On board of Spacecraft-Shenzhou No.3 (SZ-3), alloys and semiconductors, such as Al Mg2Si, Nd60Al10Fe20Co10, Pd40Ni10Cu30P20, Al-Al3Ni, GaMnSb, Bi12SiO20:Ce, and Cd0.96Zn0.04Te:Ge, were prepared. SZ-3 successfully returned to the earth on April 1, 2002. Profiting from SZ-3, great progress has been made in the researches on ma terials under microgravity in space. The quartz ampoules containing the materials grown on board of SZ-3 were shown in CFig. 1 (see the Appendix). The properties of the materials prepared on board of SZ-3 are still under investigation.     

NUMERICAL MODELLING OF VELOCITY AND TEMPERATURE DISTRIBUTIONS OF THE BUOYANCY CONVECTION EFFECT IN KNbO3 MELT

Numerical modelling of velocity and temperature fields in high-temperature KNbO3 melt of a loop-shaped Pt wire heater is carried out by using the commercial com putational code ANSYS for the mathematical solution of the governing equations.Based on the experimental boundary conditions and the Boussinesq approximation,the numerical modelling of a steady and two-dimensional model is applied to study the process under consideration of the buoyancy-driven convection condition. The result is compared with the previous experimental and theoretical data obtained in our laboratory, and the former is in agreement with the latter. Thus a theoretical guide for reasonable growth conditions is provided by studying in depth the real fluid flow effects in the crystal growth from the melt.     

一种基于北斗三号系统的GNSS-R海面干涉测高技术

GNSS-R干涉测高技术可用于中尺度海面高度观测，具有空间分辨率高、测量精度高等优势。与传统的GNSS-R本地码测高技术相比，GNSS-R干涉测高技术可以有效提升高度测量精度。虽然GNSS-R干涉测高技术已有一些研究，但是基于北斗三号的干涉测高应用还很少。本文根据GNSS-R干涉测高技术优势，针对北斗三号系统在干涉测高技术上的应用，研发了支持北斗三号的GNSS-R干涉测高接收机并描述了整体架构及实现。利用所研发的接收机进行水面干涉测高试验，首次获取了北斗三号B1和B2干涉测高波形，与传统GPS L1和北斗B1本地码测高波形进行对比。对两种方法计算出的水面高度进行对比，结果显示北斗三号干涉测高精度明显优于GPS L1和北斗B1传统本地码测高精度。      

粘弹性材料阻抗非局域特性实验验证

基于材料透射阻抗的定义阐述了粘弹性材料的局域和非局域性质,并阐述了阻抗矩阵和频响函数矩阵之间的关系.通过将声压表面力的分布离散为等效点力的方法导出了频响函数表达式.基于频响函数矩阵元素的表达式,对粘弹性材料平板进行了点力激振下振动透射的频响测量实验,同时用粘弹性有限元方法数值计算了该板的振动频率响应,实验和数值结果的一致不但验证了粘弹性材料频率响应和声阻抗的非局域特性,也说明了实验及数值方法的正确,为进一步研究打下基础.     

The Main Results and the Perspectives in the Researches at SSRT

In this report briefly presented the contemporary state of the experimental base of Radio Astrophysical Observatory (RAO) of the Institute of Solar-Terrestrial Physics (ISTP), the methodology of radioheliographic monitoring of the solar corona, the SSRT database, the RAO Web-pages, factors limiting the effective use of SSRT. Here are formulated the original results of the basic directions of the solar activity researches and the problems solutions on SSRT: (1) active regions at various development stages, morphology, modeling,signs of energy accumulation and flares buildup, forecast of powerful flares; (2) scenario, topology and the fine temporal picture of flares development, signs of primary energy release, radio emission mechanisms, scatter effects of radio emission in turbulent corona, energetic particles fluxes; (3) filaments; (4) CME with the localization of their initiation at the solar disk background, development scenario of filament activation + CME +flare; (5) coronal holes, and (6) bright coronal points.      

脉冲激光测距误差标定及不确定度分析CSCD

以脉冲激光测距机的测距误差标定为背景,通过对测距误差解析表达式的推导,给出了系统各不确定度分量对测距误差的影响,计算了信号延迟时间、探测器和激光二极管响应时间、晶振频率、大气折射率等不确定度分量。通过对某已标定激光测距机实验验证表明:该装置在500m^20 000m测距范围内,测量重复性引入的相对标准不确定度最大值为0.67m,满足该类激光测距机测量不确定度5m(k=2)的校准测试需求。因此,利用该解析表达式可以实现对脉冲激光测距误差的有效评估,这对于脉冲激光测距测试系统、脉冲激光测距机的设计具有重要的指导意义。     

Crystallization of calcium phosphate in microgravity.

Dilute solutions of CaCl2 and KH2PO4 + K2HPO4 were diffusing from either side into a mixing chamber with KCl solution. The microgravity experiment yielded aggregates of large crystals of OCP (Ca8H2(PO4)3,5H2O) and spherolites of smaller, but still visible crystals of HAP (Ca5OH(PO4)3), the stable final phase. Ground-based experiments yielded submicroscopic HAP crystals. Results of calculations of diffusion and crystal growth on the basis of previous knowledge agree well with observations.     

天宫二号碲化锌晶体生长

在天宫二号飞船综合材料实验炉六工位采用碲熔剂法生长了碲化锌晶体,生长时最高温度为800℃,以0.5mm·h-1的提拉速度向炉膛内部提拉生长晶体.飞行实验后,用相同实验参数在地面进行了对比实验.结果发现,空间样品尾部有一个非常大的橙色结晶区域（约10mm×6mm×2mm）,而地面生长样品中碲化锌晶体尺寸仅为约3mm×3mm×1mm,空间生长的碲化锌晶粒尺寸明显优于地面.空间微重力环境下,由于毛细作用,空间样品的塞子处有Te和ZnTe的外延膜生成.而地面生长的锭条在塞子处只有零星点状气相生产物.因此微重力条件有利于碲化锌晶体材料的生长.