基于一维模型的涡轮过渡流道优化设计

降低涡轮过渡流道的损失,缩短其长度,增大其径向偏移,是提高高涵道比涡扇发动机经济性和环境友好性的重要手段之一。目前研究基于所发展的一维涡轮过渡流道性能预测方法,提出了涡轮过渡流道设计的优化问题,融合单纯性优化方法,建立了一套有自主知识产权的涡轮过渡流道初步优化设计体系,用于涡轮过渡流道的快速设计。文中简要讨论了涡轮过渡流道的一维性能预测方法,给出了一维优化过程中所涉及诸多因素的确定,如几何的参数化、目标函数的确定,优化方法的选取、初步设计的建立以及优化的流程等。最后,以某实际涡轮过渡流道的优化设计为研究对象,对所发展的方法进行了验证,结果表明优化后的流道在总压损失和压升方面都较原型有了提高。通过目前的设计算例,充分确认了方法的鲁棒性和有效性。     

提高水反应金属燃料能量性能的理论分析

采用最小自由能热力计算方法,计算了不同配方水反应金属燃料的能量性能,分析了粘合剂、氧化剂、高能添加剂、金属的种类及含量对燃料能量性能的影响。计算结果表明:镁基水反应金属燃料的基础上,添加含能粘合剂(聚叠氮缩水甘油醚(PGAP)、聚3-叠氮甲基-3-甲基氧丁环(PAMMO)、聚二叠氮甲基氧丁环与四氢呋喃共聚物(PBAMO-THF))、高能金属添加剂(Al和Mg-Al合金)及增加金属含量均有利于提高燃料的燃温和理论比冲;氧化剂和高能添加剂的种类、氧粘比(氧化剂与粘合剂质量比)对燃料的燃温和理论比冲影响不明显。采用PBAMO-THF,Al分别取代端羟基聚丁二烯(HTPB)和Mg,金属含量由70%提高到80%时,燃料的理论比冲(水燃比φ=3)由4550.5 N.s/kg提高到5451.0N.s/kg。     

脉冲雷达探测中高轨道目标方法及试验

通过分析中高轨目标雷达回波信号特性,给出一种基于空间目标动力学约束的回波信号相参积累方法,介绍了信号积累模式下中高轨道目标的参数测量方法。通过对国内某型号雷达进行中高轨目标探测支路改造及相关试验,获取试验数据并对其进行分析,验证了原理的正确性和方法的可行性。     

高功率微波武器系统中的天线

文章介绍具有极高脉冲功率、很高的方向性和很低的旁瓣特性的高能微波(High Power Microwave,HPM)天线及其辐射特性。     

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).     

A fast satellite selection algorithm with floating high cut-off elevation angle based on ADOP for instantaneous multi-GNSS single-frequency relative positioning

With the Global Navigation Satellite System (GNSS) developing, the single-frequency single-epoch multiple GNSSs (multi-GNSS) relative positioning has become feasible. Since a larger number of the observed satellites make the instantaneous (single-epoch) positioning time-consuming, a proper satellite selection is necessary. Among the present methods, the satellite selection with a fixed high cut-off elevation angle (CEA) is least time-consuming. However, there is no criterion how large a fixed high CEA should be to achieve a high success rate and less time consumption. Besides, a fixed high CEA makes the number of visible satellites largely variable, which affects the success rate. Hence, a satellite selection strategy based on ambiguity dilution of precision (ADOP) is proposed. Firstly, the theoretical proof that the ADOP increases the least when removing satellites are all low-elevation-angle satellites is given, which is important to achieve the fast positioning with a high success rate. Then, the threshold $\beta$ is calculated for a different number of satellites and a given ADOP. The satellites are selected based on their elevation angles from high to low until $\beta$ of the selected satellites becomes smaller than the corresponding threshold; this method is called the extended floating CEA multi-GNSS (EF-multi-GNSS). The comparison of the single-frequency single-epoch positioning performance of the EF-multi-GNSS with the satellite selections based on a fixed low CEA (L-multi-GNSS) and a fixed high CEA (H-multi-GNSS) via the relative positioning experiments shows that: (1) the EF-multi-GNSS with a minimal number of satellites can achieve the fast positioning and a high success rate close to 100%. It can greatly reduce the time consumption of the L-multi-GNSS, by about 64.0%, by selecting 12.6 satellites of 23.4 satellites; (2) the floating CEA of EF-multi-GNSS eliminates the consideration how large a fixed high CEA should be, and a CEA larger than the fixed high CEA of the H-multi-GNSS makes it more suitable for different conditions.     

高空长航时无人机用涡扇发动机技术分析

为了研制能在高空稳定工作、且耗油率低的、高空长航时用的涡扇发动机,借助数值计算和试验数据,对此类发动机在高空工作时,其压缩系统、燃烧系统、涡轮、控制系统、润滑系统和内部空气系统所遇到的问题作了较为系统、深入的探讨和分析。结果表明,高空低Re使压缩系统、燃烧系统和涡轮性能下降,控制系统必须调整所有与飞行高度有关的参数,滑油箱压力、油泵气蚀和滑油冷却问题必须予以考虑,内部空气系统会影响冷却和封严效果。对每一个问题都提出了相应的解决办法。     

CCD光学遥感器参数选择研究

介绍了由衍射受限非相干成像系统的衍射分辨率引出的截止频率及混叠的概念. 为了对采样成像系统获得的图像质量进行量化, 使用图像质量因子(λF/P)表示探测器对光学系统线扩散函数采样的程度. 进一步分析了光学遥感器参数选择与信噪比的关系. 选择实际的焦距9 m, F 数为18 的空间光学系统, 利用ZEMAX 软件的像模拟功能, 对选择8.75 μm 和13 μm 像元尺寸的CCD 所获得的图像进行了模拟仿真. 仿真获得的结果验证了图像质量因子和信噪比对图像分辨率的影响.      

FY-3A卫星与NOOA系列卫星高能带电粒子实测结果的比较

FY-3A卫星是运行于830 km高度的太阳同步轨道气象卫星,其搭载的空间环境监测器可观测3～300 MeV的高能质子和0.15～5.70 MeV的高能电子.FY-3A卫星在轨工作期间,太阳活动处于由谷年向峰年过渡期,空间环境非常平静,探测结果显示3～300 MeV的高能质子分布主要集中在南大西洋辐射带异常区,0.15～5.70 MeV的高能电子分布区域除南大西洋异常区外,还分布在南北两极高纬区域.FY-3A与NOAA卫星测量结果反映出带电粒子强度及分布区域随投掷角变化的空间各向异性特征.本文在充分考虑了带电粒子时间、空间分布差异以及比对探测器之间自身设计差异的前提下,经过归一化处理后,首次对两颗卫星同期探测结果进行相关性分析,验证了两颗卫星相同时空条件下高能带电粒子通量分布的一致性;说明FY-3A空间环境监测器不仅具备空间带电粒子辐射监测能力,且探测结果有效可靠,可用作辐射带环境数据源的组成部分,为发展新的模型,深入研究辐射带高能粒子的分布、起源和传输等提供新的观测依据.     

太阳周期活动对低高度内辐射带高能质子的影响

利用NOAA-15卫星1998年到2011年近13年的高能质子全向通量观测资料, 分析了一个太阳活动周内, 低高度内辐射带高能质子通量的分布变化特性及其物理原因, 比较了观测结果与AP8模型的不同. 研究表明, 低高度内辐射带高能质子通量与太阳活动水平的反相关关系与磁壳参数L值及磁场B值有关; L值越低, B值越大的空间点, 其高能质子通量与太阳活动水平的反向相关性越明显. 高能质子通量随太阳活动水平的变化存在明显滞后现象, L值越高、 B值越小的空间点, 滞后现象就越明显, 滞后严重时可以达到一年左右的时间; 这种滞后现象反映出低高度内辐射带高能质子的源与损失达到平衡是一个中长期过程. 通过与AP8模型计算结果的比较分析可以看出, 利用AP8模型时, 仅考虑地磁场长期变化对质子通量的影响可能会夸大低高度内辐射带局部高能质子通量的增强.