模糊控制技术在运载火箭姿态控制中的应用

将模糊控制理论用于运载火箭的姿态控制系统设计。以俯仰通道为例，给出了模糊控制系统框图、模糊控制器的设计及其改进。仿真结果表明，所设计的运载火箭姿态模糊控制系统简单，对内外干扰具有较强的鲁棒性。     

箭载电子仪器高阻尼双层隔振技术的理论探讨及其应用

粘弹阻尼（高阻尼）双层隔振的理论基础及其在箭载仪器上的应用在文中作了介绍。通过等加速度正弦扫描振动、强度鉴定正弦扫描振动、综合环境随机振动考核证明了隔振效果显著。     

近地轨道运载火箭轨迹／总体参数一体化优化设计

在运载火箭概念设计阶段 ,总体参数的确定结合轨迹优化设计能最大程度地提高设计性能。从工程实际要求出发 ,建立了运载火箭轨迹 /总体参数一体化优化设计数学模型。确定了近地轨道的发射轨道优化设计方法 ,采用多重参数化法将轨迹最优控制问题转化为参数优化问题。针对一体化设计问题的求解要求提出了相应的组合优化算法。结果表明 ,经过一体化优化设计 ,衡量运载火箭性能的一个重要指标———起飞总质量减少了约3 5 %。该优化模型及其求解软件已经被成功地应用到工程设计中     

飞行器大姿态飞行时姿态偏差的相互转换

本文结合弹道式地地导弹和运载器稳定平台提供的测量角度,研究了姿控系统的姿态角、框架角和旋转角之间,尤其是各偏差之间的关系,为正确实现姿态信号反馈,特别是大姿态控制提供了依据。     

Effects of eccentricity of the reference orbit on multi-tethered satellite formations

The paper discusses the relevance of eccentric reference orbits on the dynamics of a tethered formation, when a massive cable model is included in the analysis of a multi-tethered satellite formation. The formations examined in this study are hub-and-spoke (HAS) and closed-hub-and-spoke (CHAS) configurations for in-plane and Earth-facing spin planes. Stability of the formations is studied by means of numerical simulation, together with the evaluation of the effects of eccentricity on tether elongation, agents relative position, and formation orientation and shape.     

火箭发射对塔架威胁情况建模与分析

首先分析了火箭在垂直起飞段横向漂移对发射塔架的影响,并建立了一组准确描述和计算运载火箭相对发射塔架横向(OT方向)漂移的数学处理模型,然后利用试验任务数据计算火箭在OT方向的漂移。所计算的横向漂移量为分析垂直起飞段火箭对塔架的碰撞威胁提供了有效的数据,为确定塔架结构的可靠性和提高发射过程的安全性提供了科学依据。     

Dynamical cartography of Earth satellite orbits

We have carried out a numerical investigation of the coupled gravitational and non-gravitational perturbations acting on Earth satellite orbits in an extensive grid, covering the whole circumterrestrial space, using an appropriately modified version of the SWIFT symplectic integrator, which is suitable for long-term ($～$120?years) integrations of the non-averaged equations of motion. Hence, we characterize the long-term dynamics and the phase-space structure of the Earth-orbiter environment, starting from low altitudes ($～$400?km) and going up to the GEO region and beyond. This investigation was done in the framework of the EC-funded “ReDSHIFT” project, with the purpose of enabling the definition of passive debris removal strategies, based on the use of physical mechanisms inherent in the complex dynamics of the problem (i.e., resonances). Accordingly, the complicated interactions among resonances, generated by different perturbing forces (i.e., lunisolar gravity, solar radiation pressure, tesseral harmonics in the geopotential) are accurately depicted in our results, where we can identify the regions of phase space where the motion is regular and long-term stable and regions for which eccentricity growth and even instability due to chaotic behavior can emerge. The results are presented in an “atlas” of dynamical stability maps for different orbital zones, with a particular focus on the (drag-free) range of semimajor axes, where the perturbing effects of the Earth’s oblateness and lunisolar gravity are of comparable order. In some regions, the overlapping of the predominant lunisolar secular and semi-secular resonances furnish a number of interesting disposal hatches at moderate to low eccentricity orbits. All computations were repeated for an increased area-to-mass ratio, simulating the case of a satellite equipped with an on-board, area-augmenting device. We find that this would generally promote the deorbiting process, particularly at the transition region between LEO and MEO. Although direct reentry from very low eccentricities is very unlikely in most cases of interest, we find that a modest “delta-v” ($\mathrm{\Delta }V$) budget would be enough for satellites to be steered into a relatively short-lived resonance and achieve reentry into the Earth’s atmosphere within reasonable timescales ($～$50?years).     

基于非开普勒轨道的高超声速临近空间飞行器自主天文导航研究

针对航天器自主导航方法不适合高超声速临近空间飞行器的问题, 研究了基于非开普勒轨道的高超声速临近空间飞行器自主天文导航方案. 论述了基于非开普勒轨道的自主天文导航机理, 通过对高超声速临近空间飞行器受力分析, 建立了动力学方程; 利用矢量倒数法则推导出空间运动方程; 设计了基于非开普勒轨道的状态模型和基于星光折射间接敏感地平的观测模型, 采用卡尔曼滤波进行了仿真验证. 仿真结果表明, 基于非开普勒轨道的高超声速临近空间飞行器自主天文导航可达到较高的位置和速度精度.      

A preliminary study of pulse-laser powered orbital launcher

An air-breathing pulse-laser powered orbital launcher has been proposed as an alternative to conventional chemical launch systems. The aim of the present study is to assess its feasibility through the estimation of its achievable payload mass per unit beam power and launch cost. A transfer trajectory from the ground to a geosynchronous Earth orbit (GEO) is proposed, and the launch trajectory to its geosynchronous transfer orbit (GTO) is computed using the realistic performance modeled in the pulsejet, ramjet, and rocket flight modes of the launcher. Results show that the launcher can transfer 0.084 kg of payload per 1 MW beam power to a geosynchronous earth orbit. The cost becomes a quarter of existing systems if one can divide a single launch into 24,000 multiple launches.     

Design of transfer trajectories between resonant orbits in the Earth–Moon restricted problem

The application of dynamical systems techniques to mission design has demonstrated that employing invariant manifolds and resonant flybys enables previously unknown trajectory options and potentially reduces the ΔV$\mathrm{\Delta }V$ requirements. In this investigation, planar and three-dimensional resonant orbits are analyzed and cataloged in the Earth–Moon system and the associated invariant manifold structures are computed and visualized with the aid of higher-dimensional Poincaré maps. The relationship between the manifold trajectories associated with multiple resonant orbits is explored through the maps with the objective of constructing resonant transfer arcs. As a result, planar and three-dimensional homoclinic- and heteroclinic-type trajectories between unstable periodic resonant orbits are identified in the Earth–Moon system. To further illustrate the applicability of 2D and 3D resonant orbits in preliminary trajectory design, planar transfers to the vicinity of L₅ and an out-of-plane transfer to a 3D periodic orbit, one that tours the entire Earth–Moon system, are constructed. The design process exploits the invariant manifolds associated with orbits in resonance with the Moon as transfer mechanisms.