一种低分辨雷达飞机目标识别方法

介绍了一种基于低分辨雷达回波序列的飞机目标识别方法。该方法把一维回波序列变换成二维轮廓像,在二维轮廓像基础上,提取到较一维回波更加稳定、有效的特征。采用神经网络做为分类器,利用所提取的特征对五类飞机目标进行识别试验,得到了较高的正确识别率。     

基于相位重合点检测技术的频标比对系统

相位重合点检测是一种高准确度测量周期性信号参数的技术,已实际应用于高准确度频率计中。介绍了相位重合点检测技术的原理及其在频标比对系统中的应用。实际工作情况证明,采用相位重合点检测技术的频标比对系统,具有电路简单,可靠性高的优点,测量分辨力达到了100 ps量级。     

压力、温度组合畸变对某发动机影响的数值研究

本文给出了组合畸变的描述参数,详细地计算和分析了组合畸变对某发动机稳定性的影响,讨论和分析了在不同组合相位和畸变强度下的影响情况。计算结果表明:当压力和温度畸变相位完全重合时,压缩系统中将产生最大的稳定裕度损失;如果适当调整压力与温度的组合畸变相位,一种畸变可能削弱另一种畸变,实际上可增加稳定裕度。     

基于水膜流动与耦合传热的翼型防/除冰计算

针对飞行器防/除冰过程中翼面上空气-水膜-冰层-机翼之间的耦合传质传热现象,建立了一种基于水膜流动与耦合传热模型的翼型防/除冰数值模拟方法.基于Myers水膜流动模型建立了防/除冰热载荷作用下翼面溢流水流动、积冰及内部温度分布的数值计算理论.对于翼型及冰层内的传热现象,利用焓理论及有限体积法建立了复杂多层结构传热的数值...     

Phase Equilibria in Nb-Si-Mo Ternary Alloys at 1 273 K and 2 073 K

Phase equilibrium in Nb-Si-Mo ternary alloys （〈37.5 at.% Si） at 1 273 K and 2 073 K is investigated by using X-ray diffraction （XRD） analysis, scanning electron microscopy （SEM） and energy dispersive spectroscopy （EDS）. The partial isothermal section at 1 273 K, which contains four single-phase regions, five two-phase regions and two three-phase regions, is basically the same as that at 1 973 K. However, when the temperature increases to 2 073 K, the three-phase region of Nbss＋ct-（Nb（Mo））sSi3＋13-（Nb,Mo）sSi3 obviously moves towards the Nb-rich comer. This suggests that Nb-Si-Mo ternary alloys remain stable at least up to 1 973 K.     

日本技术试验卫星-Ⅷ在轨运行浅析

简要介绍日本技术试验卫星-Ⅷ的概况,分析了技术试验卫星-Ⅷ的系统设计特点和在轨初始运行情况及故障,并简述了该卫星今后的运行计划。     

一种低轨星座高精度相位保持方法

针对大型低轨星座在轨运行的高精度构型保持问题,提出了一种基于极限环的高精度相位保持方法。首先,推导了实际轨道与参考轨道的平相位角偏差与半长轴偏差的关系；然后,建立了基于极限环的相位保持周期以及半长轴改变量计算方法；最后,基于推导的半长轴偏差与相位偏差的关系,提出了一种相位保持实施方法。考虑地球非球形和大气阻力的数值仿真表明：本文提出的相位保持方法能够在卫星定轨数据精度不高、数据采样间隔较大的情况下,实现低轨星座系统的高精度相位保持。     

Fast calibration of between-receiver GPS/Galileo/BDS differential phase bias with millimeter accuracy based on short baseline mode

The differential code and phase biases induced by the receiver hardware (including receiver, antenna, firmware, etc.) of the Global Navigation Satellite System (GNSS) have significant effects on precise timing and ionosphere sensing, thus deserve careful treatment. In this contribution, we propose an approach to fast fix the single-difference ambiguity to finally obtain the unbiased estimates of between-receiver differential phase bias (BR-DPB) and between-receiver differential code-phase bias (BR-DCPB) based on the short baseline mode. The key to this method is that the error sources can be significantly eliminated due to the length of the baseline is very short. At the same time, the empirical constraints and random characteristics of BR-DPB/BR-DCPB were considered, which is conducive to the resolution of single-difference ambiguity. Several sets of GNSS data (GPS L1/L2, Galileo E1/E5b, and BDS B1/B3), recorded by the short baselines in an interval of 30 s and covered a broad range of receiver/antenna types (JAVA, SEPT, LEIC, and TRIM), were used to verify the effectiveness of the proposed method. The numerical tests show that the proposed method is capable of fast fixing the single-difference ambiguity successfully within a few epochs and then providing the unbiased estimates of BR-DPB and BR-DCPB in an epoch-by-epoch manner. Experiments show that the estimated BR-DPB is in millimeter accuracy, which is of great significance for the millimeter-accuracy phase time transfer and ionospheric delay estimation. Furthermore, the calibrated BR-DPB/BR-DCPB can be treated as the known products for long-distance precise timing and ionosphere sensing based on the inter-station single-difference model.     

RadioAstron reveals super-compact structures in the bursting H2O maser source G25.65+1.05

Water masers are well-known to be variable on a variety of time scales, but only three Galactic H₂O masers are known to flare to the level of 10⁵–10⁶ Jy (${\text{T}}_{\text{B}}\sim {10}^{17}$ K): Orion KL, W49N, and the recently discovered G25.65+1.05. Recently detected flaring activity of H₂O maser in the massive star-forming region G25.65+1.05 gave us a unique opportunity to study the fine structure of H₂O maser emission in the bursting state with extremely high space VLBI angular resolution. Observation of the source was carried out with ∼9 Earth diameter space-ground baseline within the framework of the RadioAstron project. H₂O maser emission from two spectral features, including the bursting one, was detected in the experiment. Only ∼1% of the bursting H₂O maser emission was detected on the space-ground baselines: it indicates the presence of a very compact spatial structure with a size of ∼25 $\mathrm{\mu }$as, which corresponds to 0.05 AU or ∼5 solar diameters at the distance to the source of 2.08 kpc, and the brightness temperature of ∼3 × 10¹⁶ K. Analysis of the flux density as a function of the baseline length for the bursting H₂O maser feature in the source shows that most of the emission comes from an extended “halo” structure, while the core of emission is very compact and has an extreme brightness temperature. These results are in agreement with the model of interacting maser clouds considered as the likely explanation of the nature of the burst in the source. Under the assumption of such a model, the beam size of maser emission is reduced while the brightness temperatures similar to the highest observed values are produced.     

Evaluation of rapid phase clock/bias products for PPP ambiguity resolution and its application to the M7.1 2019 Ridgecrest,California earthquake

Precise point positioning with ambiguity resolution (PPP-AR) is a useful tool for high-precision geodetic and geophysical applications, while phase bias products are the prerequisite to implement PPP-AR. Wuhan University has been providing the final (the best operationally post-processing solution based) phase clock/bias products with a latency of two weeks since March of 2019, while a dedicated open-source software package PRIDE PPP-AR is released to leverage these products for high-precision positioning. In order to satisfy some both time and precision critical applications, such as rapid earthquake response, Wuhan University also released rapid (with comparable quality but with much shorter delivery latency) phase clock/bias products with a latency of less than 24 h and updated PRIDE PPP-AR in July 2019. We first introduce the phase clock/bias generation and validation schemes and the maintenance of routine products provision. Then, with 14 days (July 2 to July 15 in 2019) of GPS data collected from 146 globally distributed IGS (International GNSS Service) stations, we evaluated the positioning performance of the rapid products with respect to their final counterparts. It is found that positioning precision of PPP-AR using rapid products is comparable to that using final products, especially in kinematic positioning mode. When rapid products are used, the RMS of PPP-AR in static mode with respect to IGS weekly solutions can reach 1.7 mm, 1.8 mm and 5.5 mm in the east, north and up components, respectively. Furthermore, the RMS of epoch-wise positions with respect to daily solutions for the east, north and up components are 0.51 cm, 0.57 cm and 1.51 cm for PPP-AR with rapid products in kinematic mode. It demonstrates that the rapid phase clock/bias products can sufficiently meet the precision requirement of most geodetic and geophysical applications yet with much shorter time delay. Finally, we study the July 6th M7.1 2019 Ridgecrest, California earthquake using the rapid phase clock/bias products and demonstrate their comparable performance against the final products.