悬停状态电控旋翼桨距控制

针对改进型电控旋翼系统,首先建立了其各控制环节的数学模型,采用串级PID(proportion in-tegration differentiation)控制算法设计了悬停状态下电控旋翼桨距控制律,PID参数根据Ziegler-Nichols方法进行整定.通过仿真计算分析,初步验证了该控制算法对于桨距控制的有效性.以上述控制方法为基础,进一步开展了悬停状态下电控旋翼桨距控制的闭环试验研究,成功的实现了电控旋翼桨距幅值和相位的控制,验证了串级PID电控旋翼桨距控制算法的正确性和有效性.      

一种基于偏好MOEA的卫星地面站资源多目标优化算法

随着中国航天事业的发展,卫星地面站资源匮乏问题日益突出,需要对其进行统筹优化使用。因此,卫星地面站资源规划问题得到了广泛关注。在分析问题特点的基础上,对用户规划结果的偏好信息进行建模表达,建立了涵盖用户偏好的多目标数学规划模型,提出了基于偏好多目标进化算法的卫星地面站资源规划算法。为了进一步提升算法性能,设计了基于领域知识的启发式策略,包括：任务扩充策略、冲突消解策略以及任务缩减策略等。实验结果表明,与现有算法相比,用户偏好信息的引入能有效提升问题求解针对性,在IGD-CF （Inverted Generational Distance based on Composite Front）指标上取得了更好的效果。     

流体力学深度学习建模技术研究进展

深度学习技术在图像处理、语言翻译、疾病诊断、游戏竞赛等领域已带来了颠覆性的变化。流体力学问题由于维度高、非线性强、数据量大等特点,恰恰是深度学习擅长并可以带来研究范式创新的重要领域。目前,深度学习技术已在流体力学领域得到了初步应用,其应用潜力逐渐得到证实。以流体力学深度学习技术为背景,结合课题组近期研究结果,探讨了流体力学深度学习建模技术及其最新进展。首先,对深度学习技术所涉及的基本理论做了介绍,阐释流场建模中常用深度学习方法背后的数学原理。其次,分别对流体力学控制方程、流场重构、特征量建模和应用等几个典型的人工智能与流体力学交叉问题应用场景所涉及的深度学习技术研究进展进行了介绍。最后,探讨了流体力学深度学习建模技术所面临的挑战与未来发展趋势。     

一种非规则采样航空时序数据异常检测方法

航天器遥测数据的实时异常检测对于航天任务具有重要意义。以往方法大都考虑规则采样且缺失率较低的时序数据,然而航空时序数据具有维度大、噪声多、缺失率高、采样间隔不规则等特点,因此异常检测任务较为困难。针对非规则采样且具有缺失值的多维航空时序数据提出非规则采样多维时序数据异常检测（IMAD）算法。首先,采用带有可训练迟滞项的门控循环单元（GRU-D）对缺失值和非规则采样的时序数据进行建模;然后,采用变分自编码器建立随机性模型,学习正常时序数据的分布,从而对噪声数据具有鲁棒性;最后,利用基于极值理论的自适应阈值确定法确定合适阈值进行异常检测。结果显示,在两个真实航空时序数据集上,IMAD具有超出当前最新异常检测算法的性能;多个实验表明,IMAD在缺失率、参数以及数据集变化时,能够维持较好的异常检测效果,具有较强的鲁棒性。     

火箭橇运动计算算法优化与试验验证

对火箭橇试验系统进行了动力学分析,研究了火箭橇运动计算方法,在常规算法基础上对各参量计算方法进行改进,并引入了新的参量能量耗散阻力,进而得到优化算法。取四次不同速度的双轨橇车试验结果分别与常规算法和优化算法计算结果进行比较,得到:常规算法计算结果误差最小为7.67%,误差最大为37.91%,优化后算法计算结果误差最小为0.48%,误差最大为5.0%;取四次不同速度的单轨橇车试验结果分别与常规算法和优化算法计算结果进行比较,得到:常规算法计算结果误差最小为11.78%,误差最大为43.64%,而优化算法计算结果误差最小为0.11%,误差最大为5.31%。结果表明火箭橇运动计算优化算法相比常规算法能有效提高计算结果精度,计算结果对火箭橇试验设计具有一定工程指导意义。      

Research Advances of Solar Corona and Interplanetary Physics in China: 2012–2014

Solar transients and their related interplanetary counterparts have severe effects on the space environments of the Earth. Therefore, the research of solar corona and interplanetary physics has become the focus of study for both solar and space scientists. Considerable progress has been achieved in these aspects by the solar and space physics community of China during 2012–2014, which will be given in this report. The brief report summarizes the research advances of solar corona and interplanetary physics into the following parts: solar wind origin and turbulence, coronal waves and seismology, solar eruptions, solar energetic particle and galactic cosmic ray, magnetic reconnection,Magnetohydrodynamic(MHD) models and their applications, waves and structures in solar wind,propagation of ICMEs/shocks and their arrival time predictions. These research achievements have been achieved by Chinese solar and space scientists independently or via international collaborations.     

航天器舱体热密封结构多物理场耦合数值分析方法研究

综合考虑航天器舱体外围高超声速流动、密封带及舱体结构传热以及密封结构内部的空腔流动传热,提出航天器高温热密封结构的瞬态多物理场耦合分析方法。利用改进型Van Driest变换方法进行高超声速流动环境预测,基于高斯－赛德尔分块迭代耦合方法完成一体化耦合计算方法。采用包含不同材料结构部件的复合结构,计算了0～200 s内有无密封塞两种情况下的各部分结构的瞬态热传导过程。结果表明,密封塞的使用可显著降低空腔内的最高温度,瞬态变化情况的考虑更加准确地反映了各部分结构部件及内部空腔的温度变化情况。该文的计算方法可广泛应用于航天器热密封结构的传热特性分析,可为火箭等航天器上的高温密封部件设计提供有效的数值分析工具。     

A Simulation of the Mid-and Low-latitude Ionospheric Electric Fields

A theoretical model of ionospheric electric fields at mid- and low-latitudes is developed. In the geomagnetic dipolar coordinate system, the ionospheric dynamo equations were solved, and the ionospheric electric potential and electric field were derived respectively. Major parameters for the model inputs, such as the neutral winds, the densities and temperatures of electron, ions and neutrals, are obtained from empirical models. The global ionospheric electrical potential and field at mid- and low-latitudes derived from our model are largely in agreement with the results presented by other authors and the empirical model. Using our model, it is found that the diurnal component of the HWM93 wind mainly contributed to the formation of the vertical electric field, while the semidiurnal component mainly contributed to the zonal electric field. Finally, by adjustment of the input F region winds and conductivities, most discrepancies between our model and the empirical one can be eliminated, and it is proved that the F region dynamo is the most significant contribution to the electric fields.      

发射箱压力波传播的数值分析及试验验证

利用计算流体动力学方法建立了发射箱内燃气流场计算分析模型,对火箭弹发射时箱内压力波传播进行了数值分析,获得了箱内前后出口处的流场压力。通过合理的设计开盖压力,能可靠实现发射箱前后盖的自动开启。经飞行试验验证,数值分析结果与试验情况吻合良好,表明箱内燃气流场计算分析模型的正确性。     

Optimal two-impulse rendezvous with terminal tangent burn considering the trajectory constraints

The two-impulse orbital rendezvous problem with a terminal tangent burn between coplanar elliptical orbits is studied by considering a lower bound on perigee radius and an upper bound on apogee radius for the transfer orbit. This problem requires that two spacecraft arrive at the rendezvous point with the same arrival flight-path angle after the same flight time. The admissible range of the final true anomaly that meets the perigee and apogee constraints is obtained in closed form. The revolution number of the transfer orbit is expressed as a function of the true anomaly and the revolution numbers of the initial and final orbits. All the feasible solutions are obtained with a bound on the revolution number of the final orbit. Then, the minimum-fuel one is determined by comparing their costs. Finally, two numerical examples are provided to obtain all the feasible solutions for given initial impulse points and the optimal solution with the initial coasting arc. Numerical results show that the minimum-fuel solution for the terminal tangent burn rendezvous is close to that for the cotangent rendezvous when the rendezvous time is long enough; however, the cotangent rendezvous may not exist when the rendezvous time is short.