模型不确定的空间机器人无力传感器阻抗控制方法

针对自由漂浮空间服务机器人在轨捕获时与服务对象的碰撞问题,提出一种考虑模型不确定情况下的无力传感器阻抗控制方法.通过将不确定模型观测的接触力和神经网络对模型不确定部分辨识得到的接触力,共同作为末端执行器与服务对象抓捕点的估计接触力和阻抗控制器的反馈,使空间机器人在模型不确定和无力传感器的情况下仍能实现与服务对象的柔性接...     

空间激光通信调制技术的研究进展

空间激光通信系统具有传输速率高、体积小、质量轻、功耗低等特点,适用于卫星高速数据传输。激光通信调制技术作为空间激光通信系统的一项关键技术,是影响系统通信性能的主要因素之一。首先,介绍空间激光通信调制技术的原理及其分类,并对其优缺点做比较分析,再对激光调制的关键技术进行阐述;然后,从发展阶段与应用环境角度对国内外已报道的空间激光通信调制技术研究进展进行总结;最后,对空间激光通信调制技术的发展趋势进行展望。     

AWGN信道中一维调制与二维调制的信道容量

卫星通信和深空通信信道都可近似为加性高斯白噪声信道,所以研究这种信道中常用调制方式下的信道容量有重要意义.从香农信息论出发,推导出了一维调制和二维调制下的信道容量.在此基础上,阐明了在不同信噪比条件下应采用的调制方式,以及编码调制能够在不牺牲频谱利用率的前提下,得到编码增益的本质.讨论了无带宽约束下AM调制和PSK调制的香农限和在高信噪比条件下PSK的近似容量.      

速度对微多普勒的影响及其补偿研究

微多普勒为雷达目标识别提供了一种新的思路和方法,而目标的平动速度会影响微多普勒信息的提取.以锥体目标的进动为例来研究速度对微多普勒的影响,并提出中心法进行等效速度补偿,该方法不是先估计出速度值再对原始信号进行补偿,而是基于原始信号频谱信息进行的一种后处理.仿真结果表明该方法能有效地补偿速度.同时基于速度补偿后的频谱,提出重心法估计微多普勒的调制带宽并与中心法进行了比较,且采用最小二乘法拟合了不同信噪比下的估计误差.估计出的调制带宽可作为一种参数特征用于识别.     

基于速度积分匹配的旋转调制惯导系统动基座对准方法

卫星导航信息辅助动基座对准过程中,速度噪声会影响对准精度和快速性,制约了旋转调制惯导角秒级高精度快速对准的实现.针对这一问题,提出了一种基于旋转调制惯导速度积分匹配的快速动基座对准方法,通过建立旋转调制惯导动基座对准误差方程和卡尔曼滤波观测模型,以消除动基座对准对载机特殊运动的要求.最后,在实验室静态环境和车载环境下,分别开展了速度积分匹配和速度十位置组合导航动基座对准仿真实验.仿真结果表明,提出的速度积分匹配方法具有误差估计量收敛速度快的特点,在对准精度不降低的情况下相对组合导航匹配方式能有效缩短动基座对准时间,并能基于旋转调制惯导取消动基座对准对载机的机动需求.     

Improving aircraft aerodynamic performance with bionic wing obtained by ice shape modulation

For Unmanned Aerial Vehicles (UAVs) with limited electrical power to achieve effectively anti-/de-icing at the leading edge of the wing, a strategy of ice shape modulation was proposed. Isolated simulated ice shape pieces printed by 3D printing technology are mounted on a NACA0012 finite wing model, and its lift/drag coefficients and suction-side velocity fields are measured by the six-component force balance and the Particle Imaging Velocimetry (PIV), respectively. The ratio of the spanwise length of a single ice shape piece to chord length and the spanwise length of the non-icing area between the two adjacent single ice shape pieces are defined as dimensionless ice shape length (w/c) and dimensionless modulation ratio (w/λ), respectively. The results indicate that for a fixed w/λ, the wing lift coefficient first increases and then drops with increasing w/c, and a peak value exists when w/c is between 0.1 and 0.2. The lower the w/λ is, the higher the wing lift coefficient will be. The periodical variation of the flow separation area along the spanwise direction is attributed on the one hand to the acceleration effect of the flow field in the non-icing area which reduces the separation area, and on the other hand to the cross-flow caused by the streamwise vortices from the non-icing area to the icing area which promotes the mixing of the flow field (similar to vortex generators). The obtained modulation law is verified through flight tests and provides guidance for the use of ice shape modulation scheme for UAVs that cannot be completely anti-/de-icing under severe weather conditions.     

旋转调制下的抗晃动干扰初始对准方法

针对晃动基座下的对准精度受限于惯性器件常值误差，提出了旋转调制下的抗晃动干扰初始对准方法。首先，分析了单轴连续旋转调制技术对常值误差的补偿机理，并在此基础上建立了晃动基座下的惯性器件输出模型;其次，详细推导了基于双重积分的惯性系粗对准算法，通过惯性坐标系下的姿态更新跟踪载体实际姿态变化消除了角晃动干扰，通过对比力进行双重积分克服了线振动影响;最后，在粗对准算法基础上，进一步建立了旋转调制下的系统状态方程和量测方程，通过反馈校正的卡尔曼滤波算法实现最优估计精对准。仿真结果表明:旋转调制下的抗晃动对准方法在克服晃动干扰的同时，能够解决对准精度受限问题，有效提高了初始对准精度。     

双层梯度蜂窝吸波结构优化设计

设计了一种带蒙皮和金属底板的双层梯度蜂窝吸波结构，并利用Hashin-Shtrikman（HS）模型获得其等效电磁参数。在此基础上，以反射率低于-10dB带宽最大为优化目标，利用保收敛粒子群优化算法（Guarantee Convergence Particle Swarm Optimization，GCPSO）对四种不同排序方案的双层梯度蜂窝吸波结构进行优化设计。结果表明，入射电磁波的角度和极化方式以及吸波材料的选择、排序和厚度对双层梯度蜂窝结构的吸波性能有很大的影响；不同入射角度下TM极化时的吸波特性明显优于TE极化，在入射角为60^°时最为明显；对比四种方案优化结果显示，case 1方案由于选用损耗角较小的吸波材料充当透波层，分布于蒙皮下面，而选用损耗角较大的吸波材料作吸收层，并置于吸波结构底层，因而具有最大的优化目标函数，吸波效果最佳，且蜂窝高度仅为具有相同吸波效果的case 3方案的49.44%。因此，选择case 1方案作为本文最终优化结果。     

Pipelines vibration analysis and control based on clamps' locations optimization of multi-pump system

The violent vibration of hydraulic pipelines in aircraft may cause faults or even an accident, especially for the large aircraft with the multi-pump system because of different vibration sources and complex pipelines system. Aiming to the vibration analysis and control of the multipump system, this paper proposed the clamps’ locations optimization to minimize the system impedance at vibration frequencies. Firstly, the models of the flexible clamp and other components in multi-pump system were es...     

First measurements of periodicities and anisotropies of cosmic ray flux observed with a water-Cherenkov detector at the Marambio Antarctic base

A new water-Cherenkov radiation detector, located at the Argentine Marambio Antarctic Base (64.24S-56.62 W), has been monitoring the variability of galactic cosmic ray (GCR) flux since 2019. One of the main aims is to provide experimental data necessary to study interplanetary transport of GCRs during transient events at different space/time scales. In this paper we present the detector and analyze observations made during one full year. After the analysis and correction of the GCR flux variability due to the atmospheric conditions (pressure and temperature), a study of the periodicities is performed in order to analyze modulations due to heliospheric phenomena. We can observe two periods: (a) 1 day, associated with the Earth’s rotation combined with the spatial anisotropy of the GCR flux; and (b) $～$ 30 days due to solar impact of stable solar structures combined with the rotation of the Sun. From a superposed epoch analysis, and considering the geomagnetic effects, the mean diurnal amplitude is $～$ 0.08% and the maximum flux is observed in $～$ 15 h local time (LT) direction in the interplanetary space. In such a way, we determine the capability of Neurus to observe anisotropies and other interplanetary modulations on the GCR flux arriving at the Earth.