基于径向对称二元阵的非同向阵列测向方法

非同向阵列是指阵元指向互不相同的阵列,其在辐射源测向方面具有独特的优势,已广泛应用于电子侦察。由于多径传输、电离层折射等传播因素的影响,电子侦察面临着更多的（椭）圆极化信号,现有的非同向阵列测向方法对（椭）圆极化信号存在固有的测向偏差。研究了电磁波及天线极化对非同向阵列测向的影响机理,提出了一种基于径向对称二元阵的非同向阵列测向方法,能够测量任意极化信号的到达方向,对于非同向阵列技术的发展具有重要的意义。仿真结果对文中所提出的算法进行了验证。     

GEO非合作目标超近距相对位姿视觉测量

提出一种基于几何特征综合匹配的双目超近距相对位姿视觉测量方法。首先,将失效卫星的矩形太阳帆板作为几何特征,采用综合匹配方法实现了双目图像的高精度匹配,随后基于几何特征指标参数判别和ROI检测方法,实现了卫星太阳帆板特征点组的识别与提取,在此基础上,进一步建立了目标坐标系,通过三维重建完成了超近距阶段失效卫星的相对位姿高精度解算。最后建立了高精度双目视觉超近距相对测量实验系统,结合所提出的综合匹配算法和相对位姿解算方法,完成了动态非合作目标的相对位姿测量实验,实验结果说明所提出的方法具有较好的实时性和较高的精度。     

视觉检测中圆形标志的定位方法研究

在使用圆形人工标志的计算机视觉检测中,标志的中心定位准确度直接影响到检测的整体准确度。在利用数学形态学算法提取标志边缘的基础上,采用椭圆拟合法、灰度加权质心法、灰度平方加权质心法对标志中心进行定位,并通过实验比较了三者的定位准确度和稳定性。最后得出,在视觉检测中可采用灰度加权质心法来定位标志的中心。     

非线性效应对重力波特性的影响

通过分析二维情况下重力波波包在等温大气中非线性传播的数值模拟结果,对非线性效应对重力波特性的影响做了定量分析。分析结果表明;重力波在非线性传播过程中,一方面由于非线性作用,随着波振幅的增加,垂直波长减小,同时平流成份增加;另一方面,尽管存在非线性效应,线性重力波的色散关系与偏振关系仍然适用。     

Solar-tracking methodology based on refraction-polarization in Snell's window for underwater navigation

Underwater navigation system is an indispensable part for autonomous underwater vehicles. Due to the indiscernibility of satellite signal, however, the underwater navigation problem is quite challenging, and a satellite-free navigation scheme should be looked for. Polarization navigation, inspired by insects’ capability of autonomous homing and foraging, is an alternative solution to satellite navigation with great application potential. Underwater polarization provides an indirect sun compass t...     

About the equilibrium and stability of the magnetopause

This paper offers a model of the magnetopause based on the theory of the contact discontinuity; the boundary layer between the two states of space plasma. The structure of the magnetopause is explored for the effects of polarization, and the profiles of the polarizing electrostatic field are obtained.     

About the equilibrium and stability of non-electroneutral current sheaths

In this paper, we prove the necessity of using the Cauchy problem, i.e., initial value problem, for solving the equilibrium (steady state) current sheet. In this connection, it appears that equilibrium current sheaths exhibit structural instability.     

Off-axis irradiation and the polarization of broad emission lines in active galactic nuclei

The stokes Monte Carlo radiative transfer code has been extended to model the velocity dependence of the polarization of emission lines. We use stokes to present improved modeling of the velocity-dependent polarization of broad emission lines in active galactic nuclei. We confirm that off-axis continuum emission can produce observed velocity dependencies of both the degree and position angle of polarization. The characteristic features are a dip in the percentage polarization and an S-shaped swing in the position angle of the polarization across the line profile. Some differences between our stokes results and previous modeling of polarization due to off-axis emission are noted. In particular we find that the presence of an offset between the maximum in line flux and the dip in the percentage of polarization or the central velocity of the swing in position angle does not necessarily imply that the scattering material is moving radially. Our model is an alternative scenario to the equatorial scattering disk described by Smith et al. (2005). We discuss strategies to discriminate between both interpretations and to constrain their relative contributions to the observed velocity-resolved line and polarization.     

Exoplanetary searches with gravitational microlensing: Polarization issues

There are different methods for finding exoplanets such as radial spectral shifts, astrometrical measurements, transits, timing etc. Gravitational microlensing (including pixel-lensing) is among the most promising techniques with the potentiality of detecting Earth-like planets at distances about a few astronomical units from their host star or near the so-called snow line with a temperature in the range 0–100 ^°C on a solid surface of an exoplanet. We emphasize the importance of polarization measurements which can help to resolve degeneracies in theoretical models. In particular, the polarization angle could give additional information about the relative position of the lens with respect to the source.     

极化角对跟踪接收机相位影响分析

根据卫星通信中遇到的极化问题及其对移动地面站的影响,针对不同极化卫星间的差异,从电磁场理论中极化的定义和分类出发,给出不同极化电磁波电场信号表示方法,以某型移动卫通站天线馈源结构为例,介绍了不同状态下极化工作方式和线极化方式中线极化面调整的机理,然后结合单通道单脉冲跟踪接收机工作原理,对天线跟踪水平极化信标时线极化角与跟踪接收机相位间的关系进行了详细分析,为解决实际应用中遇到的跟踪接收机相位漂移问题提供了技术依据。