Predicting performance in manually controlled rendezvous and docking through spatial abilities

Manually controlled rendezvous and docking (manual RVD) is a challenging space task for astronauts. This study aims to identify spatial abilities that are critical for accomplishing manual RVD. Based on task analysis, spatial abilities were deduced to be critical for accomplishing manual RVD. 15 Male participants performed manual RVD task simulations and spatial ability tests (the object-manipulation spatial ability and spatial orientation ability). Participants’ performance in the test of visualization of viewpoints (which measures the spatial orientation ability) was found to be significantly correlated with their manual RVD performance, indicating that the spatial orientation ability in the sense of perspective taking is particularly important for accomplishing manual RVD.     

一种变速风力机全风速范围发电策略

由于风力机系统复杂的机械阻尼和大惯量等强非线性因素的存在,增大了控制策略设计与实现的难度。同时,对于变速风力发电系统而言,风力机的转速控制器设计是实现发电控制策略的重要环节。本文首先分析了定桨距变速风力机全风速段的发电策略,针对传统方案所存在的问题,提出了新型的控制策略,该策略在不同运行状态之间的过渡过程迅速平滑,有效降低了系统的动态载荷;其次,基于现有的风力发电系统分析了定桨距风力机的小信号模型,推导了风力机系统的传递函数,并为转速控制环设计了P ID控制器;最后,通过仿真和实验,验证了全风速段发电策略的可行性和有效性。     

三角翼大幅度俯仰运动非定常洞壁干扰实验研究

在 3m低速风洞中用两个后掠角均为 70°的大小三角翼模型进行过失速非定常运动模拟 ,两个模型外形几何相似 ,根弦比为 1∶ 2 .1 2 5。在模型运动过程中测量模型的非定常气动力和风洞洞壁上的非定常壁压。研究大小模型对非定常气动力和非定常壁压特性的影响以及模型运动的缩减频率效应和雷诺数效应。结果表明 ,非定常壁压与非定常气动力一样具有迟滞特性 ,模型越大 ,迟滞环越大。     

近地球赤道面轨道上磁性刚体卫星的混沌运动

讨论地球磁场中非自旋磁性刚体卫星在近赤道平面圆轨道上平面天平动的混沌问题.利用Melnikov方法预测出现混沌的可能性并数值验证混沌的存在性.研究表明地球磁场的周期扰动能引起卫星的混沌运动,扰动增大则混沌加强.     

TiAl金属间化合物缺口断裂性能

 TiAl合金作为准脆性材料,在其服役过程中由于缺口的存在使得断裂对缺口非常敏感,严重降低了其使用性能,因此需要研究TiAl合金在缺口作用下的断裂性能。采用带缺口的组合拉伸试样研究了温度和拉伸速率对具有近全片层组织Ti-48Al-2Cr-2Nb合金缺口断裂性能的影响。结果表明,室温下TiAl合金对缺口非常敏感,随着温度的升高,TiAl合金对缺口敏感性降低,当温度为800 ℃时,TiAl合金对缺口不敏感。TiAl合金在低温区塑性变形是通过位错滑移和变形孪晶引起的,高温下是由扩散控制的位错攀移作用引起的。研究还表明,200 ℃下拉伸速率较低时TiAl合金对缺口不敏感,当拉伸速率增加到较高时,TiAl合金对缺口很敏感。     

BOM多视图映射技术

提出了BOM多视图的概念,介绍了BOM多视图映射技术,给出并分析了BOM多视图映射的数据流程图,实现了BOM多视图数据之间的数据映射。     

无控航天器与空间碎片再入的工程预测方法研究现状

无控航天器、火箭末级以及空间碎片再入地球大气层后可能未烧尽,残存的小碎片高速撞击地面,对人类安全和生态系统构成极大威胁。提前预测其再入轨迹并采取预防措施能够有效降低地面风险。文章对无控航天器和空间碎片再入工程预测模型,包括航天器模型、动力学模型、气动热模型和烧蚀解体模型的研究现状进行跟踪与总结,也介绍了国内外有公开资料的工程应用软件,并讨论若干关键问题和进一步研究方向。     

Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan

Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5°N, 109.1°E; Geomagnetic coordinates: 178.95°E, 8.1°N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity.     

铍的激光深熔焊工艺及显微组织

为了提高铍激光焊接的熔深,对其焊接工艺进行了探索.以Nd:YAG激光作为热源,用AlSi12为钎料.采用SEM、EDS分析等手段研究了接头的显微组织、成分分布,分析了铍激光深熔焊的裂纹产生机理.研究表明:通过优化焊接工艺参数,实现铍的激光深熔焊可能性较大.     

图像法求液滴表面张力和接触角

空间流体实验具有无人操作的特殊性,需要对监控图像进行实时处理,得到目标参数.本文研究了利用照相机捕捉到的液滴灰度图像,分析求取液滴的表面张力、接触角、体积等物理参数的方法.针对液滴的灰度图像,利用边界提取、域值分割等图像处理方法,得到液滴的基本轮廓.建立基于液面像素点坐标的拉普拉斯方程,运用牛顿一拉夫逊法、龙格-库塔法、坐标轮换法等多种数值方法,对液滴的边界进行拟合,寻求最优的轮廓拟合点.根据最优的拟合点,确定液滴的物理参数.提出了利用牛顿法与一维寻优相结合的算法进行轮廓拟合的方法,并与文献[1]提出的算法进行了比较,证明了该方法具有收敛速度较快,拟合精度较高的特点.该方法是实现空间蒸发液滴热毛细对流和接触角测量实验的一项关键技术,同时也可以运用到非接触测量的实验场合.