L波段高效小尺寸功率放大器载片设计

为了应对当前市场对功率器件更低成本、更小尺寸和更优性能的要求，设计了一款工作频率为1.2～1.4GHz的高效率小尺寸氮化镓（gallium nitride,GaN）基功率放大器载片。使用有源时域负载牵引系统对GaN管芯进行在片测试并提取管芯的非线性行为模型，在先进设计系统（advanced design system,ADS）软件中利用模型进行阻抗匹配电路设计和仿真，将功率放大器端口匹配到了目标阻抗50Ω。该载片采用谐波控制技术使功率放大器附加效率提高了6%～8%，采用高介电常数的陶瓷材料将载片电路集成在8mm×8mm。实测结果显示，放大器在漏源电压28V、100us脉宽和10%占空比脉冲输入的工作条件下，在小尺寸的载体上实现了输出功率大于56W，功率附加效率大于78%的高效率指标。     

直升机高置信度中值使用飞行谱编制方法

依据直升机使用寿命分布规律,在高置信度条件下,提出了飞行谱编制的最小样本容量准则。在此基础上,采用科目统计和飞行状态分解技术,基于单机10年统计分析的方法,研究了直升机高置信度中值使用飞行谱编制原理,以此编制的使用飞行谱具有一定的置信区间,能够真实地反映直升机单机短期执行任务的分散性和整个机群长期服役的规律性,为研究直升机关键动部件的损伤与直升机定寿提供依据。     

Orbital error propagation considering atmospheric density uncertainty

Due to the influence of various errors, the orbital uncertainty propagation of artificial celestial objects while orbit prediction is required, especially in some applications such as conjunction analysis. In the orbital error propagation of artificial celestial objects in low Earth orbits (LEOs), atmospheric density uncertainty is one of the important factors that require special attention. In this paper, on the basis of considering the uncertainties of position and velocity, the atmospheric density uncertainty is also taken into account to further investigate the orbital error propagation of artificial celestial objects in LEOs. Artificial intelligence algorithms are introduced, the MC Dropout neural network and the heteroscedastic loss function are used to realize the correction of the empirical atmospheric density model, as well as to provide the quantification of model uncertainty and input uncertainty for the corrected atmospheric densities. It is shown that the neural network we built achieves good results in atmospheric density correction, and the uncertainty quantization obtained from the neural network is also reasonable. Moreover, using the Gaussian mixture model - unscented transform (GMM-UT) method, the atmospheric density uncertainty is taken into account in the orbital uncertainty propagation, by adding a sampled random term to the corrected atmospheric density when calculating atmospheric density. The feasibility of the GMM-UT method considering atmospheric density uncertainty is proved by the further comparison of abundant sampling points and GMM-UT results (with and without considering atmospheric density uncertainty).     

短波红外全天时自主天文导航技术展望

基于2微米全天巡天（2MASS）短波红外巡天点源星表,分别从白天可探测恒星分布、天空背景辐射与大气传输、传感器性能和光学系统视场大小等方面,分析了短波红外波段相对于可见光波段,在大气层内白天观星实现全天时天文导航的优势,并展望了其发展方向。     

空间低频射电天文天线材质-观测性能分析

15MHz以下的射电天文信号由于受到电离层的阻挡只能通过空间卫星平台进行观测。采用空间展开的电小天线是目前普遍的做法。就电小天线的材质-接收性能方面进行分析，构建了基于材质磁导率、电导率对后端接收机噪声影响模型。通过计算结果比对和就天线材质空间展开难易程度的综合考虑，归纳总结了不同材质对空间低频射电天文观测噪声影响以及展开难度，为新天线的研制提供了数据依据。该项工作将为下一步L1点空间天气监测卫星中的太阳射电观测载荷提供技术支持。