双组元统一推进系统加注混合比改进算法及应用

卫星双组元统一推进系统加注混合比,是确定卫星氧化剂和燃烧剂加注量的重要参数。正确地确定加注混合比可以减少卫星的呆重,增加推进剂余量和卫星寿命。文章在原有混合比计算的基础上,分析了在轨不同阶段的不同压力、温度条件下10N推力器和490N变轨发动机的流量情况和入口压力、氧化剂和燃烧剂压力变化情况,利用推力器和变轨发动机地面...     

星载蓄电池组软件V/T充电控制技术研究

蓄电池组作为整星的储能部件,其充放电循环寿命是制约整星寿命的重要因素之一。适当的充电控制手段能有效地延缓蓄电池性能的衰降,延长卫星的使用寿命。文章分析了目前基于硬件模拟电路的蓄电池电压/温度（V/T）曲线充电控制技术的特点和局限性,提出了一种采用电源控制计算机软件实现的V/T曲线充电控制方法,其针对蓄电池可能出现的开路...     

基于CDMA容量的星载多波束天线赋形分析

建立LEO-CDMA通信系统容量分析模型,给出系统容量的计算方法,从系统容量的角度出发对比分析运用遗传算法赋形得到的波束增益模型和基于二阶锥形模型的波束增益模型的系统容量。结果表明,基于二阶锥形增益模型的系统容量约为基于赋形增益模型系统容量的两倍。分析结果为多波束接收天线的系统设计及赋形方案设计提供了理论依据。     

星载天线基础结构特性对振动响应的影响分析

文章通过对星载天线振劫响应问题的分析,提出了提高设计质量和改进设计方法的建议：首先,在抽象和归类的基础上,将上／下层天线结构简化为二级隔振系统：通过对上／下层二级隔振系统分析,推导了传递函数。然后,通过改变下层结构的阻尼特性、质量特性和刚度特性,定量地分析了不同参数情况下传递函数的变化情况,最后．根据分析和计算结果,提出了一般的设计规则和建议．     

翼型表面结冰准定常数值模拟

对翼型表面的结冰过程进行了准定常数值模拟。在每个时间步长内完成网格随着壁面边界的移动而更新、周围流场和水滴撞击特性重新计算、冰形计算及壁面边界的重构工作,如此循环直至所需的结冰计算时间。采用拉格朗日轨迹追踪法获得水滴撞击特性,应用考虑壁面粗糙度影响的边界层积分法计算壁面的对流换热系数,在此基础上求解Messinger结冰热力学模型,冰层始终沿壁面外法线方向生长。对NACA0012翼型在不同环境下生成的三种典型冰形进行了预测,并与实验结果进行了比较,表明本文所述方法的有效性。     

Predictive fault-tolerant control of an all-thruster satellite in 6-DOF motion via neural network model updating

The problem of controlling an all-thruster spacecraft in the coupled translational-rotational motion in presence of actuators fault and/or failure is investigated in this paper. The nonlinear model predictive control approach is used because of its ability to predict the future behavior of the system. The fault/failure of the thrusters changes the mapping between the commanded forces to the thrusters and actual force/torque generated by the thruster system. Thus, the basic six degree-of-freedom kinetic equations are separated from this mapping and a set of neural networks are trained off-line to learn the kinetic equations. Then, two neural networks are attached to these trained networks in order to learn the thruster commands to force/torque mappings on-line. Different off-nominal conditions are modeled so that neural networks can detect any failure and fault, including scale factor and misalignment of thrusters. A simple model of the spacecraft relative motion is used in MPC to decrease the computational burden. However, a precise model by the means of orbit propagation including different types of perturbation is utilized to evaluate the usefulness of the proposed approach in actual conditions. The numerical simulation shows that this method can successfully control the all-thruster spacecraft with ON-OFF thrusters in different combinations of thruster fault and/or failure.     

基于改进FCM的北斗三频组合观测值选取

以北斗卫星导航系统三频双差为基础探讨了组合观测值及误差,针对以往采用聚类方法在研究GPS三频组合数据过程中的不足,提出了基于距离修正的增量模糊C均值算法.通过调节因子有效地修正了样本中心与聚类中心的距离,获得合理的隶属度,从而得到正确的分类;构造了基于距离修正的聚类有效性指标,自动获取最佳聚类数,避免了人为确定聚类数的不合理性;在此基础上引入增量的思想,数据增加时以原有的数据集为基础,根据阈值进行归类,不需要重新进行初始计算.通过矩阵变换法及实例验证了该方法的可行性和可靠性.     

高度-速度剖面内再入轨迹快速规划

提出一种升力式再入航天器进入稠密大气后的轨迹规划方法。在预先设定攻角剖面的前提下，利用路径约束(驻点热流、动压和过载)在高度-速度(H-V)剖面内直接获得轨迹下边界；利用终端约束确定以轨迹下边界为基准的高度增量，进而通过下边界与高度增量的加和形成满足要求的再入轨迹。其中，增量的形式选取为分段二次型函数，其大小可通过割线法快速获得。倾斜角大小可根据纵向动力学方程反解得到，其方向依据航向误差角走廊确定。通过对典型工况的仿真，结果表明所提方法能够快速规划出再入轨迹，且适应性好。     

存在干扰下的无人机中继站波束成形算法

无人机(UAV)通信具有部署快、使用灵活、通信质量好等优点,在无线通信领域具有广阔的应用前景。采用UAV作为中继站构成的增强型卫星通信网络经常受到各种干扰的影响,导致其性能急剧下降。以信干噪比(SINR)最大化为准则,UAV中继站发射功率满足要求为约束条件的优化问题的基础上,提出了一种基于最大瑞利熵的波束成形(BF)算法,得出最优权矢量。为了降低BF算法的实现复杂度,进一步提出了一种基于迫零(ZF)的次优BF算法。计算机仿真验证了这2种BF算法的有效性。     

A simple control law for reducing the effective characteristic acceleration of a solar sail

The direction and magnitude of a solar sail acceleration are strongly related. For this reason, once the characteristic acceleration has been fixed, it is not possible to modulate the acceleration in a particular direction. In this work, a semi-analytical switching control law is derived, enabling a solar sail to emulate a smaller effective characteristic acceleration (without changes in geometry or optical properties); by periodically changing the pitch (cone) angle of the sail, in average over time, the acceleration produced by the sail matches exactly (in both direction and magnitude) that of a “smaller” sail. The range in which this is possible is determined, and the limitations on this range due to the size difference is computed. The method is validated on optimal Earth-Mars trajectories.