旋转FGMs层合圆柱壳行波模态频率分析

为推进功能梯度（FGMs）材料在发动机、导弹和火箭等领域的应用，旨在研究旋转FGMs层合圆柱壳的行波模态频率。采用Voigt模型和Sigmoid体积分数描述FGMs层合圆柱壳的材料属性，考虑科里奥利力、离心惯性力、环向初应力以及热内力推导了FGMs层合圆柱壳的能量表达式。采用切比雪夫正交多项式构造位移容许函数，建立了任意边界旋转FGMs层合圆柱壳的模态频率方程，并探讨了组分含量、夹层厚度、温度梯度和弹簧刚度系数等对FGMs层合圆柱壳模态频率的影响。结果表明:夹层厚度相比Sigmoid体积分数对模态频率的变化更为敏感；高旋转短薄壁圆柱壳相比长薄壁圆柱壳对边界条件和失稳现象的影响更为敏感；轴向弹簧相比其他弹簧对模态频率的影响更大。      

Experimental study on dynamic behavior of mechanically pumped two-phase loop with a novel accumulator in simulated space environment

Mechanically pumped two-phase loop (MPTL) which is a prominent two-phase heat transfer technology presents a promising prospect in thermal control for space payload. However, transient behavior of MPTL caused by phase-change and heat sources load-on/off in simulated space environment is rarely reported. In the present study, one MPTL setup was designed and constructed, and experimentally studied. Particularly, a novel two-phase thermally-controlled accumulator integrated with passive cooling measure and three capillary structures was designed as the temperature-control device. Dynamic behavior of the start-up, temperature control, and temperature adjustment were monitored; meanwhile, thermodynamic behavior within the proposed accumulator, the operating behavior as well as the heat and mass transfer behavior between the main loop and the accumulator were revealed. The results show that the fluid management function of the capillary structures for the novel accumulator is verified. The working point of the MPTL system can be adjusted by changing the temperature control point of the accumulator and it is little influenced by external heat flux and heat sources on/off. Pressure-drop oscillations which are manifested as fluctuations of temperature and pressure can be observed after phase changing due to the compressible volume within the accumulator and the negative-slope portion of the internal pressure.     

基于运行模态的复合材料梁脱层损伤识别

为了实现复合材料结构损伤的定位与定量识别,利用传递率函数的运行模态分析方法探讨了复合材料梁无损检测方法,通过对加速度传递函数的最小二乘拟合,得到结构的模态频率和阻尼,对传递率函数矩阵奇异值分解,得到结构的振型.运用曲率模态(CMS)和曲率模态变化率(CMSI)作为损伤指标,对具有单损伤、多损伤和不同损伤程度的复合材料梁...     

空间站梦天实验舱整器动力学分析和试验研究

空间站研制过程中，获取准确的航天器主要动力学特性有重要意义，整器动力学特性测试是研制过程中一项必不可少的大型试验项目。针对空间站梦天实验舱整器动力学问题，通过建立螺栓—法兰局部连接结构的有限元模型，分析接触状态下刚度随外力的变化关系，分别计算拉压特性下的刚度量级，并采用子结构综合方法，依据部件级模态测试结果得到梦天实验舱整器的动力学特性。结果表明:将螺栓法兰连接刚度等效为双线性弹簧，结合子结构综合预示方法，梦天整器动力学特性的预示具有较高精度。通过连接结构的精细化建模和子结构综合预示，只需进行舱段级模态试验，节省了研制经费、缩短了研制周期，可为空间站及其他大型航天器的研制提供指导。     

基于视惯融合的大型空间碎片质心位置辨识

大型自由翻滚碎片的质心是在轨操作基坐标系下的不动点，也是碎片连体基下动力学参数向卫星坐标系转换的基准，对其精确识别是提高碎片动力学参数辨识精度的关键。提出基于惯性单元测量数据与双目视觉定位数据融合的大型空间碎片质心位置识别方法。基于无力矩欧拉方程，获取附着到空间碎片表面的惯性单元间转换关系，利用该转换关系对惯性单元冗余测量数据优化，再优化求解惯性单元到质心点距离；利用双目视觉获取惯性单元上标记点动态坐标，再利用惯性单元到质心点距离，基于三点定位原理识别大型空间碎片的质心位置。以加入高斯白噪声的惯性单元与双目视觉测量数据进行仿真，结果表明优化解算后惯性单元实时测量数据的误差降低到1%以下，解算的质心位置三轴误差小于0.47mm；开展了地面试验，结果表明，解算的质心位置三轴误差小于0.49mm。仿真和试验证明，该方法能够为大型空间碎片的消旋、捕获任务提供准确的数据基准。     

Statistical analysis of the occurrence rate of geomagnetic storms during solar cycles 20–24

This study examines the occurrences rate of geomagnetic storms during the solar cycles (SCs) 20–24. It also investigates the solar sources at SCs 23 and 24. The Disturbed storm time (Dst) and Sunspot Number (SSN) data were used in the study. The study establishes that the magnitude of the rate of occurrences of geomagnetic storms is higher (lower) at the descending phases (minimum phases) of solar cycle. It as well reveals that severe and extreme geomagnetic storms (Dst < -250 nT) seldom occur at low solar activity but at very high solar activity and are mostly associated with coronal mass ejections (CMEs) when occurred. Storms caused by CME + CH-HSSW are more prominent during the descending phase than any other phase of the solar cycle. Solar minimum features more CH-HSSW- associated storms than any other phase. It was also revealed that all high intensity geomagnetic storms (strong, severe and extreme) are mostly associated with CMEs. However, CH-HSSW can occasionally generate strong storms during solar minimum. The results have proven that CMEs are the leading cause of geomagnetic storms at the ascending, maximum and the descending phases of the cycles 23 and 24 followed by CME + CH-HSSW. The results from this study indicate that the rate of occurrence of geomagnetic storms could be predicted in SC phases.     

飞翼布局无人机着舰飞行动力学分析

飞翼布局无人机具有独特的气动特性,研究飞翼布局无人机着舰飞行动力学特性对设计无人机着舰控制律具有重要意义。针对飞翼布局无人机着舰下滑飞行过程,建立六自由度飞行动力学模型,并通过对着舰飞行轨迹稳定性的分析,根据飞行品质对飞行轨迹稳定性的约束,计算达到一级飞行品质要求的着舰飞行速度。通过配平计算和小扰动线性化处理,得到无人机着舰下滑运动线性模型,并分析无人机纵向和横航向的固有模态特性。结果表明,飞翼无人机着舰下滑过程中,纵向的长、短周期模态及横航向的滚转和螺旋模态收敛但收敛慢,荷兰滚模态发散。     

The global response of terrestrial ionosphere to the December 2015 space weather event

This paper investigates the ionospheric storm of December 19–21, 2015, which was initiated by two successive CME eruptions that caused a G3 space weather event. We used the in situ electron density (N_e) and electron temperature (T_e) and the Total Electron Content (TEC) measurements from SWARM-A satellite, as well as the O/N₂ observations from TIMED/GUVI to study the ionospheric impact. The observations reveal the longitudinal and hemispherical differences in the ionospheric response to the storm event. A positive ionospheric storm was observed over the American, African and Asian regions on 20 December, and the next day showed a negative storm. Both these exhibited hemispheric differences. A positive storm was observed over the East Pacific region on 21 December. It is seen that the net effect of both the disturbance dynamo electric field and composition differences become important in explaining the observed variability in topside ionospheric densities. In addition, we also discuss the T_e variations that occurred as a consequence of the space weather event.