GEO/IGSO混合区域导航星座的设计与优化算法

区域导航星座能够以较低成本和较短时间获得目标区域导航能力，且地球同步轨道是构建非极区区域导航星座的重要轨道类型。提出一种基于GEO（地球静止轨道）和IGSO（倾斜地球同步轨道）的区域导航星座设计方法。基于星下点轨迹特性构造对称星座设计参数和优化参数集，并考虑地球扁率长期摄动影响，计算星座轨道参数。以导航服务区的统计GDOP（几何精度因子）为目标函数，利用差分进化算法构建星座优化模型。以印度IRNSS的7星星座为例，仿真检验了设计和优化算法的正确性，讨论了IRNSS星座优化构型和轨道类型选取。本方法采用的对称星座设计参数少，能够提升GEO/IGSO混合区域导航星座的全局优化效率，为后续非对称星座快速提供最佳星数和构型设计。     

Evaluation of SARAL/AltiKa performance using GNSS/IMU equipped buoy in Sajafi,Imam Hassan and Kangan Ports

Performance of SARAL/AltiKa mission has been evaluated within 2016 altimeter calibration/validation framework in Persian Gulf through three campaigns conducted in the offshore waters of Sajafi, Imam Hassan and Kangan Ports, while the altimeter overflew the passes 470, 111 and 25 on 13 Feb, 7 March and 17 June 2016, respectively. As the preparation, a lightweight buoy was equipped with a GNSS receiver/choke-ring antenna and a MEMS-based IMU to measure independent datasets in the field operations. To obtain accurate sea surface height (SSH) time series, the offset of the onboard antenna from the equilibrium sea level was predetermined through surveying operations as the buoy was deploying in the onshore waters of Kangan Port. Accordingly, the double-difference carrier phase observations have been processed via the Bernese GPS Software v. 5.0 so as to provide the GNSS-derived time series at the comparison points of the calibration campaigns, once the disturbing effects due to the platform tilt and heave have been eliminated. Owing to comparing of the SSH time series and the associating altimetry 1?Hz GDR-T datasets, the calibration/validation of the SARAL/AltiKa has been performed in the both cases of radiometer and ECMWF wet troposphere corrections so as to identify potential land contamination. An agreement of the present findings in comparison with those attained in other international calibrations sites confirms the promising feasibility of Persian Gulf as a new dedicated site for calibration/validation of ongoing and future altimetry missions.     

NiCrAl/Diatomite可磨耗封严涂层制备及性能

分别利用大气等离子喷涂技术制备了Ni/Al粘结底层、火焰喷涂技术制备了NiCrAl/Diatomite可磨耗封严涂层，研究了喷涂距离、送粉速率、火焰气体总流量、喷涂角度和氧燃比等喷涂参数对生长速率和涂层硬度的影响。结果表明，在较低的氧燃比条件下（O₂∶C₂H₂<1.6），随着喷涂距离的增大，涂层生长速率逐渐下降，硬度先保持不变后逐渐上升；当O₂∶C₂H₂>1.6时，涂层的生长速率会随着喷涂距离的增大先增大后减小，硬度随之逐渐下降。随着喷枪对基体相对移动速度的增大，涂层生长速率略微下降，硬度略有上升。气体总流量的增大使得涂层的生长速率明显上升，硬度明显下降。随着送粉量的增大，涂层生长速率明显提高，硬度随之先上升后下降。     

航空发动机限寿件疲劳可靠度计算新方法

针对目前的航空发动机限寿件（ELLP）疲劳可靠性分析中的小失效概率事件以及其极限状态函数具有较强非线性的特点，提出了一种具有自更新机制的半径外自适应重要抽样（AUMCROAIS）疲劳可靠性分析方法。该方法首先利用蒙特卡罗自适应重要抽样（MCAIS）快速逼近真实设计验算点（MPP）附近，随后以近似设计验算点为中心进行极坐标抽样，并依次构造主动学习函数，对近极限状态函数和抽样半径进行最优选取，从而实现最优抽样半径的更新，通过不断的更新确定出最优抽样半径，加速失效概率计算的收敛。本方法提高了设计验算点的收敛速度同时保证了计算精度，解决了小失效概率事件以及强非线性极限状态函数可靠度计算难题，最后以某型发动机压气机轮盘为对象应用本方法，并与传统的蒙特卡罗仿真（MCS）方法、蒙特卡罗半径外自适应重要抽样法（MCROAIS）和一阶可靠性方法（FORM）进行了对比，验证了本方法的高效率、鲁棒性和仿真精度。     

基于自适应Kriging代理模型的交叉熵重要抽样法

对于复杂失效域和小失效概率耦合的可靠性分析问题，本文提出了一种交叉熵重要抽样（CE-IS）方法结合自适应Kriging （AK）代理模型的求解方法（CE-IS-AK）。所提方法基于交叉熵原理，用混合高斯模型逐步逼近最优重要抽样密度函数，并采用AK模型协助逼近过程中混合高斯模型的参数的更新，从而提高了CE-IS方法的计算效率。另外，本文还改进了CE-IS方法的收敛准则，避免了方法的冗余迭代，扩大了方法的适用范围。由于在CE-IS方法中引入了AK模型，因此，本文方法所构建的重要抽样函数在保证精度的基础上提高了效率。相较于AK-MCS方法，本文方法中引入了重要抽样的思想，因此在Kriging训练点数目基本相同的情况下，大幅缩减小失效概率计算时样本池规模，并且由于利用了混合高斯模型，因而对多失效域具有较好的适用性。算例分析也证明了本文所提方法的优越性。     

50吨级氢氧火箭发动机的设计与研制

系统性地回顾了长征五号运载火箭芯一级50t级氢氧火箭发动机YF-77的设计与研制历程。通过分析氢氧发动机的特点以及国内外氢氧发动机的发展现状，阐述了国内新一代运载火箭研发的技术路线和50t级氢氧火箭发动机的研制背景；对50t级氢氧火箭发动机的总体技术方案及其特点进行了分析与总结，并在此基础上对发动机主要组件的技术方案及其特点开展分析；对发动机热试车情况、可靠性验证情况和故障排除情况进行了分析；对50t级氢氧火箭发动机的研制情况、技术特点进行了总结，并对国内氢氧发动机和液氧/甲烷发动机的发展进行了展望。     

基于双环滑模控制的直/气复合控制系统设计

直/气复合控制导弹具有强干扰、强非线性以及强耦合等特点，传统的姿态控制器难以适用于该种复杂干扰并存的情况，文章提出了基于双环滑模控制的直/气复合控制器。首先采用有限时间收敛趋近律分别构造内外环滑模控制器，并将角速度回路的滑模变量量化为直接力指令，以解决空气舵与姿控发动机之间的耦合问题。接着使用非线性扩张状态观测器估计综合干扰，从而设计控制器补偿侧向喷流干扰及模型不确定性等综合干扰的影响。然后基于李雅普诺夫方法证明了控制系统闭环稳定，分析了干扰补偿对控制器收敛域的影响。最后仿真结果表明，该方法跟踪速度快，动态过程平稳，具有较强的干扰抑制能力，具有很强的鲁棒性。     

Effect of moderate geomagnetic storms on equatorial plasma bubbles over eastern Africa in the year 2012: Evolution and electrodynamics

Equatorial plasma bubbles (EPBs) are common features of the equatorial and low-latitude ionosphere and are known to cause radio wave scintillation which leads to the degradation of communication and navigation systems. Although these structures have been studied for decades, a full understanding of their evolution and dynamics remains important for space weather mitigation purposes. In this study, we present cases of EPBs occurrences around April and July 2012 geomagnetic storm periods over the African equatorial sector. The EPBs were observed from the Communications/Navigation Outage Forecasting System (C/NOFS) and generally correlated well to the ionospheric irregularities observed from the Global Positioning System total electron content (GPS-TEC) measurements (rate of TEC change, ROT). This study revealed that the evolution of the EPBs during moderate storms is controlled by the strength of the daytime equatorial electrojet (EEJ) currents regardless of the strength of the equatorial ionization anomaly (EIA), the latter is observed during the July storm case in particular. These effects were more evident during the main and part of the early recovery phases of the geomagnetic storm days considered. However, the evening hours TEC gradients between regions of the magnetic equator and ionization crests also played roles in the existence of ionospheric irregularities.     

Ionospheric total electron content response to annular solar eclipse on June 21, 2020

The effects of physical events on the ionosphere structure is an important field of study, especially for navigation and radio communication. The paper presents the spatio-temporal ionospheric TEC response to the recent annular solar eclipse on June 21, 2020, which spans across two continents, Africa and Asia, and 14 countries. This eclipse took place on the same day as the June Solstice. The Global Navigation Satellite System (GNSS) based TEC data of the Global Ionosphere Maps (GIMs), 9 International GNSS Service (IGS) stations and FORMOSAT-7/COSMIC-2 (F7/C2) were utilized to analyze TEC response during the eclipse. The phases of the TEC time series were determined by taking the difference of the observed TEC values on eclipse day from the previous 5-day median TEC values. The results showed clear depletions in the TEC time series on June 21. These decreases were between 1 and 9 TECU (15–60%) depending on the location of IGS stations. The depletions are relatively higher at the stations close to the path of annular eclipse than those farther away. Furthermore, a reduction of about ?10 TECU in the form of an equatorial plasma bubble (EPB) was observed in GIMs at ~20° away from the equator towards northpole, between 08:00–11:00 UT where its maximum phase is located in southeast Japan. Additionally, an overall depletion of ~10% was observed in F7/C2 derived TEC at an altitude of 240 km (hmF2) in all regions affected by the solar eclipse, whereas, significant TEC fluctuations between the altitudes of 100 km ? 140 km were analyzed using the Savitzky-Golay smoothing filter. To prove TEC depletions are not caused by space weather, the variation of the sunspot number (SSN), solar wind (V_SW), disturbance storm-time (Dst), and Kp indices were investigated from 16th to 22nd June. The quiet space weather before and during the solar eclipse proved that the observed depletions in the TEC time series and profiles were caused by the annular solar eclipse.     

绿色技术创新对企业成长绩效的影响——基于研发投入强度的调节作用

随着我国经济的高速发展,生态问题日渐凸显。通过技术创新处理好经济发展和生态效益的关系成为实现绿色发展的内在要求。本文利用94家创业板制造业上市公司2014—2017年的数据,采用广义最小二乘法对绿色技术创新、研发投入强度与企业成长绩效之间的关系进行实证分析,探讨了绿色技术创新对企业成长绩效的直接影响,并对研发投入强度的调节作用进行分析。结果显示:绿色技术创新对企业成长绩效具有显著的正向影响;研发投入强度对绿色技术创新与企业成长绩效的关系产生显著的负向调节作用。