HEDM－CMDB推进剂燃烧性能的理论预测

利用建立不久的双基系平台推进燃烧模型，对几种ＨＥＤＭ加入平台推进剂后的燃烧性能进行了理论计算。结果表明：在所计算的几种ＨＥＤＭ中，ＨＮＨＡＡ最有利于提高燃烧；ＣＬ２０报有利于降低燃烧压力指数；ＣＬ－２０作为平台推进剂的高能填实综合性能最好。     

改进的Chan-粒子滤波算法超宽带室内三维定位

针对超宽带室内定位时容易受到非视距误差的影响,导致定位精度大大下降,甚至无法准确定位的问题,提出了一种融合粒子滤波的改进Chan定位新方法。首先,在Chan定位方法中引入模拟退火算法,对到达时间差(TDOA)算法的测量值进行优化,获得初步定位的最优解;然后,采用粒子滤波对测量值进行再次优化,粒子重采样后得到的中心位置即为目标节点的精确位置。仿真和实验结果均表明,该算法能有效提高在非视距环境下超宽带室内定位的精度,较好地消除非视距误差的干扰。     

基于贝叶斯方法的HPRF雷达跟踪解距离模糊方法(英文)

高脉冲重复频率(HPRF)雷达目标跟踪需要解决距离模糊问题。本文通过把脉冲间隔数和脉冲间隔变化量作为目标的离散状态,目标的距离和径向速度作为目标的连续状态,将HPRF雷达的跟踪和解距离模糊问题转换为贝叶斯框架下的混合估计问题并且利用粒子滤波方法实现。仿真结果表明本文方法在脉冲间隔数变化时仍可以正确地解距离模糊,并且跟踪精度比多假设方法高。     

DPIV系统研制及其应用

笔者在北京航空航天大学流体力学研究所多年从事系统的PIV测试技术研究,经过科研攻关成功研制出目前国内第一套完善的实时数字式粒子图像测速(DigitalParticleImageVelocimetry)系统,实现了速度场和涡量场的实时测量,而且已经成功地应用于各项流体力学的实验测量中,其中包括:1.5M超声速喷流实验、三角翼前缘涡破裂复杂流场测量实验、大型工程水洞流场校测、绕摆动圆柱卡门涡测量实验以及锥阀管道模型和漩涡分离器内部流场测量实验等[1～3]。     

铝粉颗粒燃烧及其燃烧产物凝聚成核计算研究

在建立铝颗粒燃烧模型及其燃烧产物凝聚成核模型基础上，对铝粉燃烧所形成的Ａｌ２Ｏ３平均粒径了进行了计算研究。也对推进剂燃烧环境下铝颗粒燃烧区域中温度、燃烧产物的质量分数、过饱和度及其凝聚成核速度的变化规律进行了分析讨论。     

Hybrid methods for determining time-optimal,constrained spacecraft reorientation maneuvers

Time-optimal spacecraft slewing maneuvers with path constraints are difficult to compute even with direct methods. This paper examines the use of a hybrid, two-stage approach, in which a heuristic method provides a rough estimate of the solution, which then serves as the input to a pseudospectral optimizer. Three heuristic methods are examined for the first stage: particle swarm optimization (PSO), differential evolution (DE), and bacteria foraging optimization (BFO). In this two-stage method, the PSO-pseudospectral combination is approximately three times faster than the pseudospectral method alone, and the BFO-pseudospectral combination is approximately four times faster; however, the DE does not produce an initial estimate that reduces total computation time.     

Nightside 135.6 nm emission enhancements of mid/low latitudes during geomagnetic storms as observed by the ionosphere PhotoMeter (IPM) on the Chinese meteorological satellite FY-3D

IPM has detected nightside 135.6 nm emission enhancements over a wide latitude range, from the sub-auroral latitudes to the equatorial regions during geomagnetic storms. Our work, presented in this paper, uses the data of IPM to understand these 135.6 nm emission enhancements during of geomagnetic storms and studies the variations of total electron content (TEC) and the F₂ layer peak electron density (NmF2) in the region of enhanced emissions. Middle and low latitude emission enhancements are presented during several medium storms in 2018. The variations of both the integrated electron content (IEC) derived from the nighttime OI 135.6 nm emission by IPM and TEC from the International GNSS Service (IGS) relative to the daily mean of magnetically quiet days of per each latitude bin (30°≦geographic latitude < 40°, 15°≦geographic latitude < 30°, 0°≦geographic latitude < 15°, ?15°≦geographic latitude < 0°, ?30°≦geographic latitude < -15°, ?40°≦geographic latitude < -30°) are investigated and show that on magnetically storm day, IEC by IPM always increases, while TEC from IGC may increase or decrease. Even if both increase, the increase of IEC is greater than that of TEC. From the comparison of IEC and TEC during magnetic storms, it can be seen that the enhancement of the nighttime 135.6 nm emissions is not entirely due to the ionospheric change. The time of IEC enhancements at each latitude bin is in good agreement, which mainly corresponds to the main phase time of the geomagnetic storm event and lasts until the recovery phase. The available ground-based ionosonde stations provide the values of NmF2 which match the 135.6 nm emissions measured by IPM in space and time. The variations of NmF2 squared can characterize the variations of the OI 135.6 nm emissions caused by O⁺ ions and electrons radiative recombination. The study results show that the OI 135.6 nm emission enhancements caused by O⁺ ions and electrons radiative recombination (where NmF2 squared increases) are obviously a contribution to the measured 135.6 nm emission enhancements by IPM. The contribution accounts for at least one of all contributions to the measured 135.6 nm emission enhancements by IPM. However, where the NmF2 squared provided by ionosonde decrease or change little (where the OI 135.6 nm emissions cause by O⁺ ions and electrons radiative recombination also decrease or change little), the emission enhancements measured by IPM at storm-time appear to come from the contributions of other mechanisms, such as energetic neutral atoms precipitation, or the mutual neutralization emission (O+ + O-→2O + h? (135.6 nm)) which also occupies a certain proportion in 135.6 nm airglow emission at night.     

航天器质量特性参数的在轨辨识方法

针对高精度姿态和轨道控制要求准确已知航天器质量特性的问题,提出了基于参数解耦的最小二乘法和基于PSO的非线性优化两种方法,以辨识航天器的质量、惯量和质心位置。第一种方法将惯量与质量和质心位置解耦后分别辨识;第二种方法则将参数辨识问题转换为非线性系统的全局优化问题,同时辨识出所有参数。所提出的方法均不需要假设航天器运动足够慢,克服了以往方法将待辨识参数的耦合关系强行分离的缺点,采用辨识后的参数明显提高了航天器姿态及轨道控制性能。仿真结果验证了方法的有效性。     

关于卫星姿态确定非线性滤波算法的研究

本文探讨了利用方位矢量和陀螺速率观测信息确定卫星姿态的问题。该问题实际上是一个非线性/非高斯状态滤波问题,因此,经典的基于EKF和UKF算法的姿态滤波器有可能失败,尤其是当初始状态的先验估计不可能精确得知的情况下。近来,粒子滤波理论已经开始应用于姿态确定问题,但是,这类算法往往需要大量的“粒子”,这对有限计算能力来说是一个沉重的负担。为此,本文尝试利用双重滤波方法,在每个序贯估计过程中,将有陀螺姿态确定问题暂时分解为1个四元数估计问题和1个陀螺常漂参数估计问题。本文提出了2个双重滤波器,包括1个姿态确定双重粒子滤波器和1个姿态确定的混合型滤波器。这两者都采用一个相同的四元数粒子滤波器,但在粒子重采样和平滑处理方面,不同于近来提出的类似滤波器。至于陀螺常漂估计,双重粒子滤波器发展了一个辅助粒子滤波器,而混合滤波器中则发展了一个参数UKF滤波器。通过与经典的姿态确定滤波器的仿真比较,证实了本文新提的2个算法的有效性和优越性。
     

国外高能量密度材料与目标化合物CL—20的进展

介绍了国外高能量密度材料(HEDM)发展的新动态。以多硝基/硝胺基多环化合物和主体笼形化合物等的开发研究作为契机,HEDM发展进入了一个新的阶段。CL-20即六硝基六氮杂异伍兹烷(HNIW)是一个很有前途的多环硝胺主体笼形化合物,本文着重评述它的结构、性能、应用及合成途径。认为通过它的六氮杂前驱物体系的基团转化而引入硝基的途径是可取的。