Analysis of the Accuracy of Ballistic Descent from a Circular Circumterrestrial Orbit

The problem of the transportation of the results of experiments and observations to Earth every so often appears in space research. Its simplest and low-cost solution is the employment of a small ballistic reentry spacecraft. Such a spacecraft has no system of control of the descent trajectory in the atmosphere. This can result in a large spread of landing points, which make it difficult to search for the spacecraft and very often a safe landing. In this work, a choice of a compromise scheme of the flight is considered, which includes the optimum braking maneuver, adequate conditions of the entry into the atmosphere with limited heating and overload, and also the possibility of landing within the limits of a circle with a radius of 12.5 km. The following disturbing factors were taken into account in the analysis of the accuracy of landing: the errors of the braking impulse execution, the variations of the atmosphere density and the wind, the error of the specification of the ballistic coefficient of the reentry spacecraft, and a displacement of its center of mass from the symmetry axis. It is demonstrated that the optimum maneuver assures the maximum absolute value of the reentry angle and the insensitivity of the trajectory of descent with respect to small errors of orientation of the braking engine in the plane of the orbit. It is also demonstrated that the possible error of the landing point due to the error of specification of the ballistic coefficient does not depend (in the linear approximation) upon its value and depends only upon the reentry angle and the accuracy of specification of this coefficient. A guided parachute with an aerodynamic efficiency of about two should be used at the last leg of the reentry trajectory. This will allow one to land in a prescribed range and to produce adequate conditions for the interception of the reentry spacecraft by a helicopter in order to prevent a rough landing.     

基于羽流效应分析的航天器发动机布局设计研究

为解决由航天器姿控发动机等带来的羽流热效应问题,文章通过仿真得到了在不同的发动机布局下航天器表面的羽流热流密度分布情况,通过增大发动机的推力线角度和安装点高度,可以使得发动机羽流核心区远离航天器表面,从而降低喷流对航天器表面的加热效应。综合考虑控制力矩及推力损失、布局包络和发动机支架设计等因素,对某航天器发动机布局进行了优化设计及羽流热防护设计。     

航天材料基因工程及其若干关键技术

材料基因工程的理念和将空间环境与效应纳入到航天材料研制全流程的思路将对航天材料的开发带来颠覆性的革命。文章在对国内外材料基因组计划和航天材料需求分析的基础上,首先对航天材料基因工程的内涵进行阐述,进而对基于航天材料基因工程的航天材料研制流程进行分析,最后结合空间环境效应及材料基因工程,从计算工具、试验工具、数字化数据三个维度,提出空间多因素环境与航天材料的耦合作用机理、航天材料空间多因素环境效应等效评价方法、空间复杂使役环境下航天材料性能演化模型、航天材料空间环境效应数据库、基于材料基因工程的航天材料设计模型、航天材料研制的不确定性及优化方法等关键技术和发展方向。     

Estimate of accuracy of determining the orientation of the star sensor system according to the experimental data

The BOKZ-M60 star sensor (Unit for Measuring Star Coordinates) is intended for determining the parameters of the orientation of the axes of the intrinsic coordinate system relative to the axes of the inertial system by observations of the regions of the stellar sky. It is convenient to characterize an error of the single determination of the orientation of the intrinsic coordinate system of the sensor by the vector of an infinitesimal turn of this system relative to its found position. Full-scale ground-based tests have shown that, for a resting sensor the root-mean-square values of the components of this vector along the axes of the intrinsic coordinate system lying in the plane of the sensor CCD matrix are less than 2″ and the component along the axis perpendicular to the matrix plane is characterized by the root-mean-square value of 15″. The joint processing of one-stage readings of several sensors installed on the same platform allows us to improve the indicated accuracy characteristics. In this paper, estimates of the accuracy of systems from BOKZ-M60 with two and four sensors performed from measurements carried out during the normal operation of these sensors on the Resurs-P satellite are given. Processing the measurements of the sensor system allowed us to increase the accuracy of determining the each of their orientations and to study random and systematic errors in these measurements.     

镁铝贫氧推进剂的能量分析

利用冲压发动机热力计算程序，对镁铝中能贫氧推进剂的能量特性进行了系统研究，并探讨了高能级分对该类贫氧推进剂能量性能的影响，研究结果表明，在镁铝中能贫氧推进剂中增加镁粉含量（或减少铝粉含量）贫氧推进剂的比冲下降，在一定空燃比范围内，增加空燃比有助于提高冲压发动机的比冲。提高贫氧推进剂中ＣＬ－２０和硼粉含量，可以显著提高共能量，而采用叠氮类含能粘合剂取代惰性粘合剂时贫氧推进剂的比冲降低。     

The Use of Quaternions in the Optimal Control Problems of Motion of the Center of Mass of a Spacecraft in a Newtonian Gravitational Field: I

The problem of optimal control is considered for the motion of the center of mass of a spacecraft in a central Newtonian gravitational field. For solving the problem, two variants of the equations of motion for the spacecraft center of mass are used, written in rotating coordinate systems. Both the variants have a quaternion variable among the phase variables. In the first variant this variable characterizes the orientation of an instantaneous orbit of the spacecraft and (simultaneously) the spacecraft location in this orbit, while in the second variant only the instantaneous orbit orientation is specified by it. The suggested equations are convenient in the respect that they allow the general three-dimensional problem of optimal control by the motion of the spacecraft center of mass to be considered as a composition of two interrelated problems. In the first variant these problems are (1) the problem of control of the shape and size of the spacecraft orbit and (2) the problem of control of the orientation of a spacecraft orbit and the spacecraft location in this orbit. The second variant treats (1) the problem of control of the shape and size of the spacecraft orbit and the orbit location of the spacecraft and (2) the problem of control of the orientation of the spacecraft orbit. The use of quaternion variables makes this consideration most efficient. The problem of optimal control is solved on the basis of the maximum principle. Several first integrals of the systems of equations of the boundary value problems of the maximum principle are found. Transformations are suggested that reduce the dimensions of the systems of differential equations of boundary value problems (without complicating them). Geometrical interpretations are given to the transformations and first integrals. The relation of the vectorial first integral of one of the derived systems of equations (which is an analog of the well-known vectorial first integral of the studied problem of optimal control) with the found quaternion first integral is considered. In this paper, which is the first part of the work, we consider the models of motion of the spacecraft center of mass that employ quaternion variables. The problem of optimal control by the motion of the spacecraft center of mass is investigated on the basis of the first variant of equations of motion. An example of a numerical solution of the problem is given.     

舱压对载人航天器密封舱姿态光学敏感器安装精度影响分析

姿态光学敏感器是航天器在轨姿态控制的重要部件,其安装精度直接影响航天器的姿态控制精度。为了研究舱压对载人航天器密封舱姿态光学敏感器安装精度的影响,以某载人航天器密封舱外安装的姿态光学敏感器为研究对象,通过对其安装精度要求、安装状态与舱体变形情况的分析,提出了一种敏感器在设计阶段布局的分析方法。在地面进行了模拟充压试验,验证了分析方法的有效性。根据分析和试验结果在型号后续设计中进行了相应的布局改进,改进结果满足了敏感器安装精度要求并经过了飞行试验验证。     

航天器新型高密度排插型DC10电缆安装技术

以互联网卫星上首次使用的新型高密度排插型电缆组件为研究对象,介绍了集成式排插型电连接器的制造技术要求和工作原理,从电连接器结构分析出发,研究影响该类型电缆的安装因素。首次提出了新型高密度排插型电缆的安装方法,阐述了该类型电缆的弯曲半径要求、绑扎要求、紧固力矩值要求和使用专用工装的拆卸方法。经过分系统的实际在轨性能测试验证,该安装技术可以显著降低新型高密度排插型电缆组件在大通量、高饱和度信号传输状态下性能下降的现象,成功解决了该类型电缆在卫星狭小空间下的安装与拆卸难题,提高了该类型电缆在卫星狭小空间内的安装精度和分系统的在轨可靠性,为该新型高密度排插型电缆组件的安装在后续卫星批量应用提供了技术指导和工艺基础。     

寻求一片纯洁的天空——《受活》的一种解读

《受活》这部作品以写实和荒诞的笔调,在历史和现实中回环往复,书写了历史与现实中存在的乌托邦幻想与冲动,以及这些乌托邦行为给底层人们带来的苦难,并通过对人物心灵的剖析透视了乌托邦梦想的困境。在对残疾人与圆全人两个世界的对比中,作者肯定了受活人的生存状态,表达了对那种自由自在以及纯洁的心灵世界的向往与追求。     

Multipole Models of the Earth's Magnetic Field

To develop a mathematical model of rotational motion of an artificial satellite about its center of mass under the action of various forces (magnetic, Lorentz, etc.) caused by the geomagnetic field, it is necessary to know the induction of the Earth's magnetic field (EMF) as a function of the radius vector of a given point in the near-Earth space. Because the EMF possesses a complex structure and the above-mentioned functional dependence is unavailable in explicit analytic form, a set of approximate models of the EMF should be used. The simplest such model—a right dipole (aligned with the axis of rotation)—does not enable one to reveal in detail the influence of diurnal EMF rotation on the rotational motion of a satellite. The next EMF approximation—an inclined magnetic dipole—does not suffer from the above-mentioned drawback. However, it is shown that not all corrections to the magnetic induction of the EMF of the same order of magnitude are taken into account in the course of transformation from the model of aligned dipole to the model of inclined dipole. So, to develop the EMF model accurately accounting for the absence of axial symmetry of the EMF with respect to the axis of diurnal rotation of the Earth, in general, the effect of the quadrupole component of the geomagnetic potential on the EMF induction (and, probably, even the components of higher orders) must be taken into consideration. By using the International Geomagnetic Reference Field IGRF-2000, the multipole models of the EMF, corresponding to quadrupole, octupole, and higher-order approximations, were constructed and studied in this work. The EMF potential is expressed in terms of its multipole tensors. As a result, projections of the induction and induction gradient of EMF in the center of mass of the satellite onto the axes of the orbital coordinate system can be written in convenient and concise form. The expressions for the first four multipole tensors through the known geomagnetic constants are found. A method for estimating the reliability of these models is put forward, and the regions of applicability of the quadrupole and octupole models are drawn on the plane of orbital parameters.     

Synthesis of a combined system for precise stabilization of the Spektr-UF observatory: II

The paper presents the second part of the results of search studies for the development of a combined system of high-precision stabilization of the optical telescope for the designed Spectr-UF international observatory [1]. A new modification of the strict method of the synthesis of nonlinear discrete-continuous stabilization systems with uncertainties is described, which is based on the minimization of the guaranteed accuracy estimate calculated using vector Lyapunov functions. Using this method, the synthesis of the feedback parameters in the mode of precise inertial stabilization of the optical telescope axis is performed taking the design nonrigidity, quantization of signals over time and level, and errors of orientation meters, as well as the errors and limitation of control moments of executive engine-flywheels into account. The results of numerical experiments that demonstrate the quality of the synthesized system are presented.     

Optimization of the Flight of a Spacecraft with a Solar Sail from the Earth to Mars with a Perturbation Maneuver near Venus

The trajectories of the fastest flight of a spacecraft (SC) with a solar sail from the Earth's sphere of activity to the Martian sphere of activity including the section of a perturbation maneuver near Venus are investigated. The planetary spheres of activity are assumed to be point-like; i.e., the maneuver section and the initial and final positions of the SC coincide with the corresponding positions of the planets. The initial velocity of the SC is assumed to be equal to the Earth's velocity, so that no leveling of the velocities of the SC and Mars in the final point of the flight is required. The perturbation maneuver is considered as a jump of the heliocentric velocity of the SC at the point of its contact with Venus, which does not change the magnitude of its Venus-centric velocity. The orbits of planets are assumed to be circular and coplanar; the SC trajectory lies at the plane of these orbits. The sail is planar with a specularly reflecting surface. The trajectories of optimum flights are determined as a result of solving the boundary value problem of the Pontryagin maximum principle. The families of solutions to this problem depending on the initial angular positions of Venus and Mars are constructed by the method of continuation over a parameter.     

降落伞特性对伞舱系统运动稳定性的影响

建立了伞舱系统刚性连接和弹性连接时的数学模型,针对联盟号飞船回收系统进行了动力学仿真。分析了降落伞侧向力系数、吊带长度、降落伞和载荷质量比以及吊带性质对伞舱系统运动稳定性的影响,其结论可为伞舱回收系统的设计提供参考。     

多辐射器航天器热控流体回路布局的(火积)耗散分析

为了优化多辐射器航天器热控流体回路布局，提高流体回路的散热效率，降低流体回路温度，本文基于(火积)理论，分别对多个辐射器串联和并联的流体回路布局的散热进行了分析。结果表明，排散相同热量时，流体回路的流体与管路壁面之间的温差均匀性越好，流体回路散热过程(火积)耗散越小，系统散热过程越优。进一步，对于2个辐射器的情况，分别对辐射器设置了不同的空间辐射加热热流，对辐射器的流体回路布局方式进行了比较。结果表明，辐射器与流体回路串联时，系统散热性能要优于两者并联，系统的流体温度水平最低，结果与(火积)理论分析的预测完全一致。研究结论对多辐射器的航天器热控流体回路设计具有指导意义。     

利用连续推力的人工太阳同步轨道设计方法

针对人工太阳同步轨道的设计方法进行研究,通过施加法向连续推力调整升交点赤经（RAAN）变化率。首次推导了升交点赤经在变方向推力作用下的周期摄动平均值的精确计算公式,解决了已有近似方法对相关轨道参数的取值范围存在限制的问题,并给出了对应的轨道倾角周期摄动平均值计算公式。在分析J2项摄动对升交点赤经影响的基础上,给出了所需的法向连续推力幅值和一个轨道周期内对应的速度增量的计算方法。通过数值仿真,校验了计算公式的正确性,分析了实现人工太阳同步轨道的连续法向推力对轨道倾角的影响,给出了连续推力幅值随轨道参数的变化规律,并且提出了未来工程任务的应用建议。     

航天用纳米流体流动与传热特性的实验研究

研究航天用纳米流体流动与传热特性。测量了不同粒子体积份额的航天用纳米流体雷诺数500~4000范围内的管内对流换热系数和摩擦阻力系数,详细讨论了雷诺数和纳米粒子体积份额对纳米流体对流换热系数和摩擦阻力系数的影响,分析了航天用纳米流体的强化传热性能。实验结果表明,在液体中添加纳米粒子增大了液体的管内对流换热系数,增加了液体的传热效果,粒子的体积份额是影响纳米流体对流换热系数的因素之一,在相同雷诺数条件下,纳米流体的对流换热系数随粒子体积份额的增加而增大。与原液体工质相比,航天用纳米流体的流动阻力系数稍有增大,纳米流体的流动阻力系数不随纳米粒子的体积份额而变化。与航天用纳米流体对流换热系数的增加相比,纳米流体流动阻力系数增大的程度极小,验证了纳米流体强化传热技术应用于航天器热控系统的可行性。     

电路板工装结构设计及其振动传递特性研究

针对印制电路板环境应力筛选试验要求,为减小夹具对试验结果的影响,提出以电路板尺寸、筛选效率以及固有频率等为约束的电路板工装设计优化方法,并以某型电路板为例进行电路板工装设计与迭代优化;继而开展模态仿真分析验证了工装设计的有效性;研究设计工装振动特性并固化电路板环境应力筛选测试方案,采用设计工装及固化方案完成电路板随机振动环境应力筛选试验。结果表明:所设计工装的一阶固有频率高于试验规定频率上限,满足工装夹具刚度特性要求。通过合理装夹和调整传感器布局等可使得电路板安装位置加速度功率谱密度曲线及均方根值满足GJB 1032A相关要求。     

Microscope in orbit calibration procedure for a test of the equivalence principle at 10(-15)

The scientific objectives of the MICROSCOPE space mission impose a very fine calibration of the on-board accelerometers. However the required performance cannot be achieved on ground because of the presence of high disturbing sources. On-board the CHAMP satellite, accelerometers similar in the concept to the MICROSCOPE instrument, have already flown and analysis of the provided data then allowed to characterise the vibration environment at low altitude as well as the fluctuation of the drag. The requirements of the in-orbit calibration procedure for the MICROSCOPE instrument are demonstrated by modelling the expected applied acceleration signals with the developed analytic model of the mission. The proposed approach exploits the drag-free system of the satellite and the sensitivity of the accelerometers. A specific simulator of the attitude control system of the satellite has been developed and tests of the proposed solution are performed using nominal conditions or disturbing conditions as observed during the CHAMP mission.     

固体火箭超燃冲压发动机补燃室构型的影响分析

针对不同补燃室结构参数对固体火箭超燃冲压发动机补燃室掺混燃烧性能的影响进行研究,分析各级燃烧室的长度与扩张角度对补燃室性能的影响。采用基于密度的二阶迎风格式对补燃室掺混燃烧进行模拟,湍流模型和燃烧模型分别采用SST k-ω模型和涡团耗散模型。结果表明,提高燃烧效率与降低总压损失是相互矛盾的;燃烧效率随燃烧室长度的增加而增大,随燃烧室扩张角度的增加而减小;总压恢复系数随燃烧室长度的增加而减小,随燃烧室扩张角度的增加而增大;一级燃烧室的结构参数对燃烧效率与总压恢复系数的影响最大。当补燃室的总长与出口面积一定时,以发动机的总体性能参数作为补燃室构型的优化目标,对一、二级燃烧室长度与一、三级燃烧室扩张角度进行优化。     

收拢压紧柔性太阳翼电池片应力影响因素研究

在压紧机构压紧力以及发射阶段加速度工况载荷共同作用下,收拢压紧状态的柔性折叠式太阳翼的太阳电池板上电池片的应力应满足力学强度要求。文章采用有限元方法对电池片应力主要影响因素,包括聚酰亚胺泡沫布局和厚度、聚酰亚胺泡沫力学性能、盖板结构及埋件形状等进行计算分析;总结降低收拢压紧状态下柔性太阳翼压紧点附近电池片压应力的主要来源途径,为柔性折叠式太阳翼的工程研制提供设计分析思路。