某固体火箭发动机点火启动过程三维流场一体化仿真

以某固体发动机的燃烧室和喷管为一体化研究对象,采用三维流场控制方程,应用有限体积法计算了发动机点火启动过程中燃烧室和喷管内燃气的流场特性。发动机药柱上的着火点最初出现在药柱星角尖上,然后向四周扩展;在药柱点火初期,燃气压力波先于火焰峰到达喷管;随着燃烧室内燃气压力升高,压力沿轴向分布逐渐平缓;当喷管进口压力与出口背压比达到某一值时,喷管扩张段内出现一道激波,随着压力比的升高,激波最终移出喷管,燃气流速在喷管出口处达到最大值。     

三维编织细编穿刺炭/炭复合材料拉伸与压缩性能及试件尺寸效应研究

通过对三维编织细编穿刺炭/炭复合材料的Z向和XY向进行的拉伸、压缩宏观实验,观测了不同载荷形式下和不同几何尺寸的试件的破坏模式和断口形貌,得到了材料在拉伸、压缩载荷下不同的破坏机理及材料的力学性能与试件几何尺寸的相关性。研究表明,材料Z向拉伸破坏时为平断口,XY向拉伸破坏时为台阶状断口,压缩载荷作用下Z向和XY向都为与受力方向成45°的剪切型破坏,Z向和XY向的压缩强度随试件的几何尺寸的变化具有相同的变化趋势,但Z向变化趋势较XY向更明显。所获结论为进一步进行该材料的刚度和强度预报以及强度准则的建立奠定了必要的实验基础。     

纳米NdCoO3对小球粘接高燃速推进剂燃烧性能的影响

采用盐助溶液燃烧法制备了平均粒径为10 nm、分散性良好的钙钛矿型纳米NdCoO3。用DSC考察了不同质量分数的纳米NdCoO3对AP和双基粘接剂热分解的影响,研究了纳米NdCoO3对小球粘接高燃速推进剂燃烧的催化作用。结果表明,随纳米NdCoO3催化剂质量分数的增加,催化效率先增大后减小,在质量分数为3%时催化效率最佳,此时AP高温分解峰温大幅降低,双基粘接剂的分解峰温也得到降低,二者的表观分解热增大。同时,对应的小球粘接高燃速推进剂燃速较高,压强指数较低。     

某固体火箭发动机药柱上三维裂纹扩展的判定

采用三维更新Lagrangian格式固相控制方程和线性粘弹材料本构方程,应用非线性有限元法对某固体火箭发动机药柱星角上含有横向贯穿裂纹的药柱进行了三维应力、应变分析,采用三维J积分理论计算了裂纹缝线上各积分点上的J积分.J积分沿着裂纹缝线呈现中间高、两端低的分布趋势,缝线中间部位的J积分值最大,此处最易扩展;根据J积分判据,确定了药柱星角上含有横向贯穿裂纹的发动机安全工作时的最大裂纹深度.     

北斗三号系统PPP-B2b信号定位服务模型及性能分析

给出了PPP-B2b信号定位的观测模型和随机模型,详细阐述了PPP-B2b增强改正模型和参数估计模型,并进行了静态和动态定位实验。结果表明：对于单系统,在30min的收敛时间内,北斗三号定位精度可以达到水平0.118m(静态)、0.176m(动态),高程0.208m(静态)、0.423m(动态)以内,GPS定位精度可以达到水平0.113m(静态)、0.163m(动态),高程0.206m(静态)、0.377m(动态)以内;对于北斗三号/GPS双系统,在20min的收敛时间内,定位精度可以达到水平0.092m(静态)、0.122m(动态),高程0.158m(静态)、0.312m(动态)以内。无论是收敛性还是定位精度,均能满足北斗三号精密单点定位服务指标的要求。     

First spaceborne demonstration of BeiDou-3 signals for GNSS reflectometry from CYGNSS constellation

The full constellation of Chinese Global Navigation Satellite System (GNSS) BeiDou-3 has been deployed completely and started fully operational service. In addition to providing global Positioning, Navigation and Timing (PNT) services, the BeiDou-3 satellites transmissions can also be used as the sources of illumination for Earth Observation (EO) with a bistatic radar configuration. This innovative EO concept, known as GNSS reflectometry (GNSS-R), allows to measure the Earth surface characteristics at high resolution via the reflected L-band radar signals collected by a constellation of small, low cost and low Earth orbiting satellites. For the first time in orbit, earth reflected BeiDou-3 signal has been detected from the limited sets of raw data collected by the NASA’s Cyclone GNSS (CYGNSS) constellation. The feasibility of spaceborne BeiDou-3 reflections on two typical applications, including sea surface wind and flooding inundation detection, has been demonstrated. The methodology and results give new strength to the prospect of new spaceborne GNSS-R instruments and missions, which can make multi-GNSS reflectometry observations available to better capture rapidly changing weather systems at better spatio-temporal scales.     

基于Mn3+浓度和形貌控制的高性能LiNi0.5Mn1.5O4正极材料

为了改善高电压镍锰酸锂(LiNi_(0.5)Mn_(1.5)O_4)材料的电化学性能,提出利用退火热处理过程调控Mn~(3+)含量和材料形貌来制备LiNi_(0.5)Mn_(1.5)O_4正极材料。LiNi_(0.5)Mn_(1.5)O_4材料的电性能是材料结构、形貌等多因素影响的结果。退火热处理有助于Mn~(3+)氧化成Mn~(4+),实现Mn~(3+)含量调控。退火后材料的空间结构由Fd3m向P4_332转变,且具有微米级多面体形貌,有效提高了循环稳定性和放电平台。研究表明:700℃退火保温15 h合成的材料在20 C下具有118 mAh·g~(-1)放电比容量,循环100次容量保持率提高到92.8%。因此,通过优化Mn~(3+)含量、控制材料形貌可以实现高性能LiNi_(0.5)Mn_(1.5)O_4材料制备。     

Periodic attitude motions along planar orbits in the elliptic restricted three-body problem

A way to improve the accuracy of the three-body problem model is taking into account the eccentricity of primary attractors. Elliptic Restricted Three-Body Problem (ER3BP) is a model for studying spacecraft trajectory within the three-body problem such that the orbital eccentricity of primaries is reflected in it. As the principal cause of perturbation in the employed dynamical model, the primaries eccentricity changes the structure of orbits compared to the ideal Circular Restricted Three-Body Problem (CR3BP). It also changes the attitude behavior of a spacecraft revolving along periodic orbits in this regime. In this paper, the coupled orbit-attitude dynamics of a spacecraft in the ER3BP are exploited to find precise periodic solutions as the spacecraft is considered to be in planar orbits around Lagrangian points and Distant Retrograde Orbits (DRO). Periodic solutions are repetitious behaviors in which spacecraft whole dynamics are repeated periodically, these periodic behaviors are the main interest of this study because they are beneficial for future mission designs and allow delineation of the system’s governing dynamics. Previous studies laid the foundation for spacecraft stability analysis or studying pitch motion of spacecraft in the ER3BP regime. While in this paper, at first, initial guesses for correction algorithms were derived through verified search methods, then correction algorithms were used to refine calculated orbit-attitude periodic behaviors. Periodic orbits and full periodic solutions are portrayed and compared to previous studies and simpler models. Natural periodic solutions are valuable information eventuate in the longer functional lifetime of spacecraft. Since the problem assumption considered in this paper is much closer to real mission conditions, these results may be the means to use natural bounded motions in the actual operational environment.     

低轨卫星的北斗反射信号海洋覆盖分析

北斗系统作为我国自行研制的导航系统，具有独特的混合星座特性，其反射事件在海洋上的空间分布和覆盖性能的研究成果较少。针对上述问题，模拟了北斗三号（Beidou System 3，BDS3）以及全球定位系统（Global Positioning System，GPS）空间星座，模拟不同性能参数的低轨接收卫星，在此仿真系统的基础上，计算反射事件在各仿真场景下的海洋覆盖率以及同时发生反射事件的卫星数量。结果表明：BDS3与GPS相比具有更大的反射事件海洋覆盖率，覆盖性能更优；仿真周期7天与1天相比,前者卫星产生的反射事件海洋覆盖率约为后者5倍；低轨道卫星（Low Earth Orbit,LEO）轨道高度越高，天线波束角度越大，反射事件海洋覆盖率越大；3颗LEO卫星下同时发生反射事件卫星数的平均值约为单颗LEO卫星的3倍。可通过设计多星组网来提高反射事件海洋覆盖率。研究结果对星载反射技术海洋遥感应用方面有一定的参考价值。     

Inter-satellite calibration of FengYun 3 medium energy electron fluxes with POES electron measurements

We perform an L-shell dependent inter-satellite calibration of FengYun 3 medium energy electron measurements with POES measurements based on rough orbital conjunctions within 5?min?×?0.1?L?×?0.5 MLT. By comparing electron flux data between the U.S. Polar Orbiting Environmental Satellites (POES) and Chinese sun-synchronous satellites including FY-3B and FY-3C for a whole year of 2014, we attempt to remove less reliable data and evaluate systematic uncertainties associated with the FY-3B and FY-3C datasets, expecting to quantify the inter-satellite calibration factors for the 150–350?keV energy channel at L?=?2–7. Compared to the POES data, the FY-3B and FY-3C data generally exhibit a similar trend of electron flux variations but more or less underestimate them within a factor of 5 for the medium electron energy 150–350?keV channel. Good consistency in the flux conjunctions after the inter-calibration procedures gives us certain confidence to generalize our method to calibrate electron flux measurements from various satellite instruments.