空间站实验舱柔性电池翼约束释放机构设计与验证

柔性太阳电池翼国内首次在中国空间站成功应用，是空间站系统最复杂、难度最大的机电产品之一，而约束释放机构作为柔性太阳电池翼系统的关键构成，用于实现太阳翼上升段压紧保护和在轨段解锁释放，其成败直接影响航天器任务成败。基于任务需求，本文介绍了柔性电池翼约束释放机构的构成、工作原理、详细设计以及仿真验证和在轨应用情况，分析其技术特点及关键技术。地面验证及在轨飞行试验验证了约束释放机构设计的正确性与合理性，为我国航天器多点大面积可重复压紧及解锁方面提供了一种新颖且可靠的解决方案。     

旋转对固体火箭发动机两相流点火过程影响仿真研究

为研究高速旋转对内外燃管型装药固体火箭发动机凝聚相点火瞬态过程的影响规律，应用计算流体动力学（CFD）流体计算软件，使用用户定义函数（UDF）编程接口建立固体火箭发动机点火模型，对旋转条件下发动机凝聚相点火过程进行模拟。将数值计算结果与地面旋转实验内弹道进行对比分析，验证数值模型的正确性。计算结果表明：①点火药燃气颗粒因旋转做离心运动，大量粒子聚集在燃烧室头部上端，部分粒子附着在发动机壁面，且停留时间较长。②点火药燃气颗粒占比从20%增加到40%，点火压力峰值降低3.93%，发动机转速的升高会造成内弹道平衡压力升高，但点火压力峰会逐渐降低，且峰值出现时间发生延迟，转速达到15 000 r/min时点火压力峰消失。③转速增大，点火颗粒与推进剂传热增大，火焰传播期减小，但燃气填充期和点火延迟增大，点火药燃气颗粒占比为20%时，转速为15 000 r/min较静止条件下点火延迟增加了23.76%。     

Attitude control actuator scaling laws for orbiting solar reflectors

The rapid evolution of in-orbit manufacturing will enable the fabrication of low-cost, large-scale space structures. In particular, the use of 3D printing technologies will remove traditional payload constraints associated with launch vehicles, due to fairing size and launch loads, thus allowing the construction of larger and lighter structures, such as orbiting solar reflectors. These structures will require efficient attitude control systems, able to provide the necessary torque for maneuvers and to counteract perturbations, such as gravity gradient and solar radiation pressure. In this paper, a top-level overview of actuator performances for orbiting solar reflectors is provided, and scaling laws associated with the required actuator mass and input power are developed. For each class of actuator, upper bounds on the maximum size of the structure which can be effectively controlled are presented. The results can also be extended to other classes of large planar Earth-pointing structures such as solar power satellites, solar sails, or large antennae.     

New insights from cross-correlation studies between solar activity indices and cosmic-ray flux during Forbush decrease events

Observed galactic cosmic ray intensity can be subjected to a transient decrease. These so-called Forbush decreases are driven by coronal mass ejection induced shockwaves in the heliosphere. By combining in situ measurements by space borne instruments with ground-based cosmic ray observations, we investigate the relationship between solar energetic particle flux, various solar activity indices, and intensity measurements of cosmic rays during such an event. We present cross-correlation study done using proton flux data from the SOHO/ERNE instrument, as well as data collected during some of the strongest Forbush decreases over the last two completed solar cycles by the network of neutron monitor detectors and different solar observatories. We have demonstrated connection between the shape of solar energetic particles fluence spectra and selected coronal mass ejection and Forbush decrease parameters, indicating that power exponents used to model these fluence spectra could be valuable new parameters in similar analysis of mentioned phenomena. They appear to be better predictor variables of Forbush decrease magnitude in interplanetary magnetic field than coronal mass ejection velocities.     

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.     

Novel orbit-attitude combination mode for solar power satellites to reduce mass and fuel

Solar power satellite receives great attention because it can release the energy crisis and environmental problems in the future. However, the launch and maintenance costs are tremendous due to the large system mass and large fuel consumption to counteract space perturbations. To reduce mass and fuel, a novel quasi-Sun-pointing attitude in Sun-frozen orbit is proposed. The Sun-frozen orbit has a nonzero eccentricity vector that always points towards the Sun. The quasi-Sun-pointing attitude is a periodic solution of the Sun-pointing attitude angle. Although about 3 % electricity must be given up because of the variation of Sun-pointing attitude angle, little control action is required to deal with the solar radiation pressure and gravity-gradient torque. The algorithm to obtain initial conditions is proposed. The influences of system parameters and structural flexibilities are studied. Simulation results reveal that the quasi-Sun-pointing attitude in Sun-frozen orbit dramatically reduce fuel consumption, the dry mass, and complexity of the control system. In addition, structural vibration is hardly induced by the gravity-gradient torque. Thus, the bending stiffness as well as the mass of the supporting structure can be reduced.     

搅拌摩擦加工调控镁合金组织与耐腐蚀性能的发展现状与趋势

近年来，航空航天领域轻量化进程发展迅速，镁合金在其中扮演着越来越重要的角色。然而，镁合金耐腐蚀性不佳的特点制约了镁合金的应用范围。本文综述了搅拌摩擦加工技术调控含第二相镁合金耐腐蚀性能的研究现状，从动态再结晶和加速第二相破碎、固溶两个角度，论述了搅拌摩擦加工调控镁合金组织的基本原理，并分析了搅拌摩擦加工改善含粗大第二相镁合金耐腐蚀性的原因，为改善含粗大第二相镁合金的耐蚀性提供了技术途径和研究方向。     

载人航天器太阳翼多姿态输出能力建模及分析

载人航天器太阳翼在轨运行期间除正常对日定向转动外，根据飞行任务要求可能需要工作在α轴水平归零或垂直归零等特殊状态。在特殊工作模式下，太阳入射角和太阳翼的输出能力变化曲线更加复杂。建立太阳入射角与轨道角、太阳高度角、β轴转角等变量的数学模型，分析太阳入射角的变化规律，并结合光照区时长，建立太阳翼在轨输出能力的预测模型。与实际飞行数据相比较，表明该模型可较为准确地评估特殊工作模式下太阳翼的输出能力，可用于在轨整舱能量平衡分析，为飞行任务计划安排提供参考。     

临近空间太阳电池组件热力学特性仿真分析

临近空间飞行器依靠搭载的柔性太阳电池组件和储能电池组构成的能源系统,可在临近空间长期飞行和驻留,完成地面观测、无线通信、军事侦察等任务,因而成为各国航天航空领域发展的热点之一。由于太阳电池组件能量转化效率只有20%左右,大部分太阳光能量吸收后转化为热。这部分热传导到高空气球内部,将造成内部气流紊乱,增加高空气球姿态控制难度,而温度升高引起的热应力甚至可能破坏柔性太阳电池组件。本文通过计算机模拟太阳组件在高空气球蒙皮上的工作条件,建立组件结构模型及热传递数学模型,仿真得到电池组件实际工作时的温度场和应力场分布情况,对高空气球供电组件的结构优化、工作状态的掌握具有指导意义。     

磁洁净太阳电池电路技术进展与关键技术分析

随着重力、电磁场等科学探测任务需求的日益增强，对航天器整器的磁洁净度要求日益严格，尤其是光照条件下太阳电池电路的磁洁净度。本文基于国内外重大科学探测型号任务，梳理了国内外磁洁净太阳电池电路技术的发展历程、实现方式以及型号应用情况，并从正面布局、背面线缆以及基板厚度方向等方面系统分析了实现磁洁净太阳电池电路的关键技术:选用低磁材料、镜像对称布局与自由端线缆控制、补偿电缆，为后续磁洁净太阳电池电路技术的进一步突破提供参考。