运载火箭起飞噪声环境缩比模型试验方法

基于相似理论建立缩比模型试验相似准则,提出了火箭发动机喷流声场试验预示方法的流程。通过缩比模型系留点火试验,根据几何相似、喷流参数相似、发射环境相似来预示起飞噪声环境,在国内首次给出了运载火箭表面的噪声环境的空间相关特性,结果表明预测结果与遥测数据之差小于1.5 dB,校验了缩比模型方法的有效性。缩比模型方法对于我国新一代运载火箭的起飞噪声环境预示、噪声载荷设计、地面试验具有重要意义。     

一种基于时间梳技术的高频正弦信号相位差测量方法

本文研究了一种基于时间梳原理的高频正弦信号相位差测量方法,给出了时间梳原理的数学模型,并详细分析了其特点,并将此原理首次应用于高频信号的数据采集中,可以用低频和被测信号构建一种高频等效采样技术,可以在不满足乃奎斯特采样定理下,对被测两路正弦信号进行同步采样,避免了高频信号采样的高采样率,结合多重互相关技术,实现了对高频正弦信号的相位差的高精度测量,实验结果表明本文算法对高频信号对高频正弦信号的相位差测量具有很高的测量精度,尤其在低信噪比下也有较高的测量精度,具有较高的工程实用价值。     

大涡模拟进口合成湍流方法

进口瞬时湍流脉动条件直接影响大涡模拟的精度。对比研究了更适合工程应用的合成涡和合成谱方法,并通过考虑进口速度时间相关和随机数的概率密度分布,对合成谱方法进行改进。对零压力梯度平板湍流模拟结果的对比表明:不同湍流合成方法得到的合成湍流均存在发展为真实湍流的过渡过程;考虑进口湍流脉动的时间相关有助于合成湍流更快地发展为真实湍流,需要的流向距离更短;合成谱方法采用正态分布系数优于均匀分布,改进的合成谱方法优于常规合成谱方法。     

伴流速度对平行喷口射流影响的数值研究

采用大涡模拟方法计算研究平行喷口出口马赫数为0.9,伴流速度比分别为0.1、0.3和0.5时的喷射流场特性。计算时采用高精度的数值模拟方法,并结合Smagorinsky亚网格尺度模型。考察了流场统计平均特性、脉动特性以及射流流场中涡结构的发展演变过程,结果表明:伴流速度的增大使得势流核长度变长,减缓了空间剪切层的发展,转捩延迟。喷射流场速度分布具有自相似性,而湍流强度的分布则不具有相似性。通过分析剪切层中轴向速度脉动、径向速度脉动、压力脉动在空间任意两点上的时空相关性,发现随着伴流速度的增大,脉动量在空间上的相关性减弱,而脉动量向下游的传递速率增加。该研究结果为进一步揭示伴流速度对喷流声场的影响提供基础。     

Microstructural characterization and mechanical behavior analysis of 7075-T6 aluminum subjected to simulated lightning strikes

Aircrafts damages caused by lightning strikes have been known since the early days of aviation. However, the physical effects on the aircraft structure are still being investigated. This work seeks to evaluate the lightning strike effects in the aluminum alloy 7075-T6. Samples were submitted to lightning strike simulation in laboratory and the damages evaluated through characterization techniques. Ultrasound and profilometry tests have shown material loss to 0.272 mm depth in the damaged region. In addition, it was detected the material accumulation occurrence in the damage vicinity of the region. Below the damage, it was found a region where metallurgical changes were identified. The tensile and microhardness tests results have shown reduction in the percentage elongation and hardness increasing in the material affected by lightning. These results are corroborated by the X-Ray Diffraction (XRD) and Rietveld Method (red line) that indicated an increasing in dislocation density and micro-deformation in the material matrix. Optical microscopy results have shown the presence of microcracks on the normal and cross-section surface of the samples damaged. The Energy Dispersive X-Ray Spectroscopy (EDXS) and Electron Backscattered Diffraction Test (EBSD) found coarse intermetallic phases and precipitates compounds with dimensions greater than 1 μm in length. They were responsible for nucleation of the microcracks that propagate along the material grain boundaries.     

地基伪卫星系统多址测距误差的校正算法

相对于卫星导航,地基伪卫星与接收机距离较近,测距中不涉及电离层传播等误差,易实现高精度测距和定位。但由于地基伪卫星位置固定,在信号连续发射模式下伪卫星信号间的多址干扰(MAI)会引起相对恒定的测距误差,针对地基伪卫星系统这一特点,提出一种基于反馈串行干扰抵消(SIC)的测距算法。首先对全部伪卫星信号进行捕获跟踪和功率估计,然后通过串行干扰抵消算法降低强功率伪卫星信号对期望测距信号的干扰,通过反馈模式进一步提高干扰抵消算法的性能。仿真结果表明,该方法可有效改善地基伪卫星系统强远近效应区域内的测距性能,不考虑其他误差下在强远近效应区域内基于码环可将伪卫星测距性能从10 m以上降低到约0.3 m。     

Search for high-proper motion objects with infrared excess

The possibility of interstellar migration has been theorized during the past thirty years in the form of “Dysonships” that, using non-relativistic propulsion systems, are able to colonize the Galaxy in a relatively short time compared to the age of the Galaxy and consequently penetrate inside our solar system too. Observational evidence of this can be potentially obtained using the present state of the art of telescopes and related sensors, by following aimed searches and an expanded SETI protocol. Some transient and unrepeated radio signals recorded during standard SETI observations might be due to the transit of high-proper motion artificial sources of extraterrestrial origin, which are expected to show a very weak optical emission, a strong infrared excess and occasional high-energy bursts in the X and Gamma-ray wavelength ranges. Such artificial sources might show an interest to Earth by sending probes to visit it: such a possibility can be investigated scientifically as well.     

Accelerating NLTE radiative transfer by means of the Forth-and-Back Implicit Lambda Iteration: A two-level atom line formation in 2D Cartesian coordinates

State-of-the-art methods in multidimensional NLTE radiative transfer are based on the use of local approximate lambda operator within either Jacobi or Gauss–Seidel iterative schemes. Here we propose another approach to the solution of 2D NLTE RT problems, Forth-and-Back Implicit Lambda Iteration (FBILI), developed earlier for 1D geometry. In order to present the method and examine its convergence properties we use the well-known instance of the two-level atom line formation with complete frequency redistribution. In the formal solution of the RT equation we employ short characteristics with two-point algorithm. Using an implicit representation of the source function in the computation of the specific intensities, we compute and store the coefficients of the linear relations J=a+bS$J=a+\mathit{bS}$ between the mean intensity J and the corresponding source function S. The use of iteration factors in the ‘local’ coefficients of these implicit relations in two ‘inward’ sweeps of 2D grid, along with the update of the source function in other two ‘outward’ sweeps leads to four times faster solution than the Jacobi’s one. Moreover, the update made in all four consecutive sweeps of the grid leads to an acceleration by a factor of 6–7 compared to the Jacobi iterative scheme.     

Tropospheric wet refractivity tomography using multiplicative algebraic reconstruction technique

Algebraic reconstruction techniques (ART) have been successfully used to reconstruct the total electron content (TEC) of the ionosphere and in recent years be tentatively used in tropospheric wet refractivity and water vapor tomography in the ground-based GNSS technology. The previous research on ART used in tropospheric water vapor tomography focused on the convergence and relaxation parameters for various algebraic reconstruction techniques and rarely discussed the impact of Gaussian constraints and initial field on the iteration results. The existing accuracy evaluation parameters calculated from slant wet delay can only evaluate the resultant precision of the voxels penetrated by slant paths and cannot evaluate that of the voxels not penetrated by any slant path. The paper proposes two new statistical parameters Bias and RMS, calculated from wet refractivity of the total voxels, to improve the deficiencies of existing evaluation parameters and then discusses the effect of the Gaussian constraints and initial field on the convergence and tomography results in multiplicative algebraic reconstruction technique (MART) to reconstruct the 4D tropospheric wet refractivity field using simulation method.     

基于伪相关函数的BOC无模糊跟踪性能分析

BOC(Binary-Offset-Carrier)调制广泛应用于全球导航卫星系统中,但由于BOC自相关函数的多峰导致传统码跟踪环路存在模糊性。伪相关函数(Pseudo Correlation Function, PCF)方法在本地采用两个特殊的参考信号和非线性处理以获得无模糊的相关函数。根据一种PCF方法本地参考波形设计的充分条件,推导了其无模糊函数的数学形式,并着重分析了其跟踪和抗多径性能与本地参考波形的关系。仿真结果表明：该PCF方法解决了跟踪模糊问题,且随着参考信号的宽度因子增加,其跟踪精度逐步改善;该PCF方法对于中长延迟多径干扰抑制能力较好,宽度因子为0.5或1时,其多径误差最小。