一种时间欠采样实时频率和二维角估计方法

提出了用均匀平行线阵和阵元输出信号的时间延迟估计时间欠采样来波频率、方位角和仰角的方法.该算法在DFT波束空间使用PRO-ESPRIT方法,实现频率无模糊估计,完成来波信号频率和角度的估计.频率间接估计算法是先估计数字频率,然后用数字频率求模拟频率,其估计方差比直接估计算法的方差要小几个数量级.仿真实验表明了算法的有效性.     

C/C-Cu复合材料的烧蚀形貌和烧蚀机理

以PAN预氧化纤维整体毡为增强体,经碳化、等温CVI致密化后制备多孔的C/C复合材料预制体,利用气体压力浸渗法将Cu引入C/C预制体中制备C/C-Cu复合材料。采用氢氧(H2-O2)焰考核C/C-Cu复合材料的烧蚀性能,经扫描电镜和电子能谱对不同烧蚀区域的微观结构和成分进行分析,结果表明:预制体密度为0.96 g/cm3的C/C-Cu复合材料的线烧蚀率和质量烧蚀率分别为4.75μm/s、0.223 mg/s,烧蚀性能优良;其烧蚀表面具有不同的宏观形貌,在烧蚀中心区产生了明显的凹坑,主要烧蚀机制为C/C预制体的氧化和铜基体的机械冲刷;烧蚀过渡区聚集了大量的铜基体,其烧蚀机制为Cu的热氧化和机械冲刷;烧蚀边缘区材料表面变黑,主要因为C/C的氧化。为了提高C/C-Cu的烧蚀性能,需要发挥C/C预制体的"钉扎"作用,阻止Cu在高温下被气流冲刷而发生流动。     

一种低复杂度的Multi-h CPM相干解调算法及FPGA实现

多调制指数连续相位调制（Multi-h Continuous Phase Modulation,Multi-h CPM）是一种恒包络调制,具有多个周期出现的调制指数,因此其频谱效率和功率效率比单调制指数CPM更高,但其接收机的复杂度也随之增加。本文在倾斜相位（Tilted Phase,TP）的基础上采用频率脉冲截断（Frequency Pulse Truncation,FPT）和状态空间分割（State Space Partition,SSP）相结合的方法来降低多调制指数连续相位调制的复杂度,使相位状态由512降低到16,理论损耗约为0.8 dB。同时,对降低复杂度的解调算法在现场可编程门阵列（Field Programmable Gate Arrays, FPGA）上进行了验证。仿真和在线测试的误码率曲线接近理论分析曲线,和常用的128状态解调算法相比,资源消耗降低了约59%。     

Comprehensive data reduction package for the Immersion GRating INfrared Spectrograph: IGRINS

We present a Python-based data reduction pipeline package (PLP) for the Immersion GRating INfrared Spectrograph (IGRINS), an instrument that covers the complete H- and K-bands in one exposure with a spectral resolving power of 40,000. The reduction steps carried out by the PLP include flat-fielding, background removal, order extraction, distortion correction, wavelength calibration, and telluric correction using spectra of A type standard stars. As the spectrograph has no moving parts, the PLP automatically reduces the data using predefined functions for the processes of order extraction, distortion correction, and wavelength calibration. Before the telluric correction of the target spectra, the intrinsic hydrogen absorption features of the standard A star are removed with a Gaussian fitting algorithm. The final result is the flux of the target as a function of wavelength. Users can customize the predefined functions for the extraction of the spectrum from the echellogram and adjust the parameters for the fitting functions for the spectra of celestial objects, using “fine-tuning” options, as necessary. Presently, the PLP produces the best results for point-source targets.     

遥测伪周期时间序列子序列异常检测算法

针对现有异常检测算法用于伪周期时间序列异常序列检测时易造成误差累积,导致序列周期与特征值上显著差异的不足,文章以卫星遥测伪周期时序数据为对象,综合两种常规分段方法的优势,提出了最大周期窗宽内基于极值的模式子序列分段算法。在此基础上,给出了一种基于均序列动态生成模型的子序列异常检测方法（AnomalySubsequenceDetectionmethodbasedonOptimizedSequenceModel,ASD_OSM）,并采用2次四分位距准则（DoubleQuantilerangescriterion,2Q准则）设置距离检测门限阈值,将超出阈值的序列判定为异常序列。某航天器传感器遥测子序列异常检测试验结果表明,提出的检测方法能够有效减少漏判,提高卫星遥测伪周期数据异常序列检测的准确性。     

基于编队控制的自适应HELLO更新算法

在无人机(UAVs)编队自组织网络中,针对无人机之间位置信息更新周期不合理,从而导致编队控制不稳定和控制开销过大的问题,提出一种基于无人机编队控制的自适应HELLO更新算法。该算法应用编队控制稳定性理论推导出无人机组成期望编队的控制延时上限,结合该延时上限和编队运动状态自适应地设定HELLO更新周期。仿真结果表明,本文提出的算法与固定HELLO更新周期算法相比,既能保证在组编控制过程的稳定性,又能实时维护稳定阶段的链路,并且显著减少网络中不必要的控制开销。      

GEO编队空间机器人系统交会方法

针对地球静止轨道（GEO）上被服务航天器的远距离和非合作特点,提出一种高自主、高协同、多任务的编队空间机器人在轨服务系统方案,实现对非合作目标的自主交会接近。首先,分析GEO卫星轨道约束力小的轨道特征和非合作的信息交互特征,给出由操作空间机器人和监视空间机器人组成的编队在轨服务系统,设计交会接近相对测量分系统以及在轨服务飞行任务;接着,给出典型远距离交会接近的多视线相对导航方法与多冲量相对制导律;最后,进行远距离交会任务仿真校验,结果表明编队空间机器人交会接近方法是有效的。     

考虑气膜冷却的涡轮静叶三维优化

为研究气冷涡轮叶片设计的特点,搭建了一个可以对采用气膜冷却的气冷涡轮叶片进行全三维优化的平台,该平台可在有冷气喷射的条件下对叶片进行多目标优化.优化平台中采用11参数法对叶片进行造型.针对该造型方法和优化设计的要求对优化变量的选取和优化策略以及优化目标的设定进行了一定的探讨,采用多岛遗传算法对优化问题进行寻优.采用该平台对某航空涡轮第一级静叶进行了优化.由于对不同目标进行了加权处理,所以随着优化目标侧重点的不同,优化方案的叶型呈现出不同特点,其气动效率和冷却效果均有所改善.     

Preparation of the Biochip experiment on the EXPOSE-R2 mission outside the International Space Station

Biochips might be suited for planetary exploration. Indeed, they present great potential for the search for biomarkers – molecules that are the sign of past or present life in space – thanks to their size (miniaturized devices) and sensitivity. Their detection principle is based on the recognition of a target molecule by affinity receptors fixed on a solid surface. Consequently, one of the main concerns when developing such a system is the behavior of the biological receptors in a space environment. In this paper, we describe the preparation of an experiment planned to be part of the EXPOSE-R2 mission, which will be conducted on the EXPOSE-R facility, outside the International Space Station (ISS), in order to study the resistance of biochip models to space constraints (especially cosmic radiation and thermal cycling). This experiment overcomes the limits of ground tests which do not reproduce exactly the space parameters. Indeed, contrary to ground experiments where constraints are applied individually and in a limited time, the biochip models on the ISS will be exposed to cumulated constraints during several months. Finally, this ISS experiment is a necessary step towards planetary exploration as it will help assessing whether a biochip can be used for future exploration missions.     

Prebiotic significance of extraterrestrial ice photochemistry: detection of hydantoin in organic residues

The delivery of extraterrestrial organic materials to primitive Earth from meteorites or micrometeorites has long been postulated to be one of the origins of the prebiotic molecules involved in the subsequent apparition of life. Here, we report on experiments in which vacuum UV photo-irradiation of interstellar/circumstellar ice analogues containing H(2)O, CH(3)OH, and NH(3) led to the production of several molecules of prebiotic interest. These were recovered at room temperature in the semi-refractory, water-soluble residues after evaporation of the ice. In particular, we detected small quantities of hydantoin (2,4-imidazolidinedione), a species suspected to play an important role in the formation of poly- and oligopeptides. In addition, hydantoin is known to form under extraterrestrial, abiotic conditions, since it has been detected, along with various other derivatives, in the soluble part of organic matter of primitive carbonaceous meteorites. This result, together with other related experiments reported recently, points to the potential importance of the photochemistry of interstellar "dirty" ices in the formation of organics in Solar System materials. Such molecules could then have been delivered to the surface of primitive Earth, as well as other telluric (exo-) planets, to help trigger first prebiotic reactions with the capacity to lead to some form of primitive biomolecular activity.