提高静压气浮陀螺加表K0、K1项精度的工艺研究

本文通过对影响静压气浮陀螺加表K0、K1项精度的因素分析,从加表及其重要组件的工作原理、结构特点、工艺过程等方面展开研究,总结出经过工艺试验及生产过程验证提高加表K0、K1项精度的关键技术,提高了加表验收合格率。     

用CST软件仿真替代部分卫星RM测试的可行性研究

环境减灾-1A、1B卫星采用CST-MWS软件完成了RM星仿真分析,快、好、省地完成了天线分系统设计验证任务。文章通过某卫星全向天线CST-MWS软件分析结果与RM测试结果的比较,表明软件分析结果的准确性满足RM验证的要求,验证了环境减灾-1A、1B卫星RM星仿真结果的正确性。进而也论证了软件仿真替代部分RM测试的可行性。     

行星际激波对地球磁层的压缩效应分析

2004 年11月9日WIND飞船探测到一个典型的行星际激波. 激波前行星际磁场为持续约50 min的弱南向磁场, 越过激波面, 磁场发生北向偏转且太阳风动压脉冲增强. 在此强动压脉冲增强结构作用下, 磁层被压缩至一个很小的区域. 激波作用于磁层时引起地球同步轨道 各区域高能粒子通量的响应, 但是不同磁地方时的高能粒子通量的响应不同, 表现出双模式扰动, 即在晨昏两侧各能段的电子和质子通量显著增强, 在子夜侧发生类似于亚暴的无色散粒子注入现象. 扰动从向阳面传输到背阳面, 向阳面粒子通量最先增强, 随后背阳面靠近晨昏两侧, 粒子通量开始增强, 最后子夜侧粒子通量表现出无色散高能粒子注入的特点. 另外, 在靠近正午侧, 质子通量先于电子通量发生响应, 在子夜侧电子通量则先于质子通量发生响应. 利用位于向阳面正午两侧的GOES-10 和 GOES-12卫星观测数据发现, 激波作用于磁层时靠近晨侧的磁场变化表现出简单压缩效应, 而靠近昏侧的磁场变化则显然不同, Bx分量减弱, Bz分量几乎减为零, 而By分量则显著增强. 此外, 位于近地磁尾低纬尾瓣区的TC-1卫星观测到激波触发的尾瓣SI现象.     

嫦娥一号卫星紫外月球敏感器

探月工程是我国航天领域的又一项重大工程项目,嫦娥一号卫星是探月工程的第一步。嫦娥一号卫星首次采用了一种全新的光学姿态敏感器——紫外月球敏感器,实现在卫星环月飞行期间的姿态测量任务。紫外月球敏感器是一种以月球为姿态参考源的大视场成像式光学姿态敏感器,本文介绍其工作原理、功能与组成以及在轨飞行试验的相关情况。     

Preliminary Scientific Results of Chang'E-1 Lunar Orbiter: Based on Payloads Detection Data in the First Phase

Chang'E-1 lunar Orbiter was launched by Long March 3A rocket from Xichang Satel-lite Launch Center at 18:05BT(Beijing Time) Oct.24,2007.It is the first step of its ambitious three-stage moon program,a new milestone in the Chinese space exploration history.The primary science objectives of Chang'E-1 lunar orbiter are to obtain three-Dimension(3D) stereo images of the lunar surface,to analyze the distribution and abundance of elements on the surface,to investigate the thickness of lunar soil,evaluate helium-3 resources and other characteristics,and to detect the space environment around the moon.To achieve the above four mission objectives,eight sets of scientific instruments are chosen as the payloads of the lunar orbiter,including a CCD stereo camera(CCD),a Sagnac-based interferometer spectrometer(ⅡM),a Laser Altimeter(LAM),a Microwave Radiometer(MRM),a Gamma-Ray Spectrometer(GRS),an X-ray spectrometer(XRS),a High-Energy Particle Detector(HPD),and two Solar Wind Ion Detectors(SWID).The detected data of the payloads show that all payloads work well.This paper introduces the status of payloads in the first phase and preliminary scientific results.     

氟橡胶-金属胶粘剂的研究

针对氟橡胶与金属的粘接难题,制备改性Chemlok 607,OG,OG’和OGs四种胶粘剂,与国内合神FA-1、国外Chemlok 607胶粘剂进行对比研究。结果表明,这四种胶粘剂用于未硫化氟橡胶与金属粘接时拉剪强度均远大于FA-1和Chemlok 607。改性Chemlok 607胶粘剂较好地解决了硅烷类胶粘剂与金属粘接性不好的问题。OG,OG’和OGs胶粘剂均可直接用于未硫化氟橡胶与金属的粘接,也可用于硅橡胶的粘接,是氟橡胶与金属粘接用的优良胶粘剂,目前已试用于汽车同步环中氟橡胶与金属的粘接。通过热失重分析(TGA)研究表明,OG,OG’和OGs胶粘剂固化物具有较高的耐热性及热稳定性。二氨基二苯砜(DDS)固化时会与氟橡胶在粘接界面处生成配位键,改善与氟橡胶的粘接性能,提高粘接强度。     

某小型涡扇发动机增压级设计与试验验证

采用经过试验验证的一维方案设计程序包以及与轴对称流设计程序相匹配的任意中弧线叶片造型程序,运用三维计算与一维、二维气动设计相结合的方法成功地完成了某小涡扇发动机增压级气动设计,并且单独设计和加工内涵两级增压级进行了试验验证,试验结果表明,该增压级具有宽广的高效率区和高喘振裕度,设计结果与试验结果吻合较好.      

嫦娥一号卫星飞行事件的系统级FMEA

嫦娥一号卫星系统级FMEA采用从上到下的分析方法,对飞行事件中可能发生的故障,以及故障发生的原因、故障影响和在轨补偿措施等进行了分析;对嫦娥一号卫星系统级FMEA的特点、工作流程和分析步骤等几方面进行了阐述;并总结了嫦娥一号卫星系统级FMEA结果和工作体会,为进一步开展系统级FMEA研究和应用提出了建议。     

耐高温复合材料在火星探测器着陆器减速伞筒盖结构上的应用

针对火星探测器着陆巡视器减速伞筒盖结构在轨运行耐温度交变、辐照等空间环境和再入过程耐温度冲击性能需求,重点开展了筒盖复合材料耐温匹配性、力学性能、耐空间环境性能以及制件成型工艺研究。结果表明,选用J-168-1胶黏剂、J-245胶黏剂及T300/QY8911复合材料制备的试件通过各项性能试验考核,均能满足筒盖结构的设计指标要求。筒盖产品力学性能稳定,成型工艺可行性良好,最高瞬时使用温度可达200℃,经历空间环境模拟后力学性能保持率均在80%以上,耐高温、耐空间环境性良好。产品已成功装星发射,并在着陆巡视器落火阶段成功弹出分离,圆满完成使命。     

Spatial asymmetry in topside ion density and vertical E × B plasma drift velocity within 75°E–95°E

The ion density measured by the Ionospheric Plasma and Electrodynamics Instrument (IPEI) on board the ROCSAT -1 over the 75°E and 95°E meridian at 600km altitude has been utilized to examine the latitudinal and longitudinal distribution within the Indian sector, in particular, the north-south and east-west asymmetries of the equatorial ionization anomaly (EIA). A longitudinal gradient in ion density at 600?km higher towards 95°E develops during the noontime and afternoon hours when the EIA is at its peak. The density gradient persists till evening hours when pre-reversal enhancements occur. The vertical E?×?B plasma drift velocity measured simultaneously by ROCSAT -1 for the same space-time configuration has also been studied. In addition to diurnal, seasonal and solar activity variations in E?×?B drift velocity, the longitudinal gradient is also observed. The EIA at the altitude of 600?km peaks at different latitudes and are mostly asymmetric about the magnetic equator. From midnight till 0800 LT, the ion density across the equator is nearly uniform in the equinoxes. But in the solstices, the density exhibits a north-south gradient. In the June solstice, density is higher in the northern hemisphere and decreases gradually towards south. The gradient in density reverses in December solstice. Normally, the EIA peaks within 1200 LT and 1600 LT while around 2000 LT, pre-reversal enhancement of ionization occurs affecting the EIA evening structure. The strength of the EIA also exhibits seasonal, year-to-year and hemispheric variations. The longitudinal asymmetry of drift velocity along 75°E and 95°E longitude sectors is the contributing factor behind the observed longitudinal asymmetry in ion density. Significant positive correlation between the strength of the EIA and E?×?B drift is observed in both longitudes.