金属载体上线天线阻抗与辐射特性的矩量法研究

用线网格模拟金属载体表面，应用矩量法求出天线及载体网格上的电流分布，据此研究在该金属载体影响下的天线特性，在计算阻抗矩阵元素时，利用了非对称正弦偶极子辐射场的精确表达式，并采用了直接复数积分，简化了计算公式，本文给出了几种金属载体上线天线的阻抗与辐射特性的计算结果，它们与有关文献上的数据或实验结果一致，最后计算了一种舰船简单模型上两根线天线的远区辐射场及它们的自阻抗与互阻抗。     

Spectra and time variability of black-hole binaries in the low/hard state

We propose a jet model for the low/hard state of galactic black-hole X-ray sources which explains the energy spectra from radio to X-rays and a number of timing properties in the X-ray domain such as the time lag spectra, the hardening of the power density spectra and the narrowing of the autocorrelation function with increasing photon energy. The model assumes that (i) there is a magnetic field along the axis of the jet, (ii) the electron density in the jet drops inversely proportional to distance, (iii) the jet is “hotter” near its center than at its periphery, and (iv) the electrons in the jet follow a power-law distribution function. We have performed Monte Carlo simulations of Compton upscattering of soft photons from the accretion disk and have found power-law high-energy spectra with photon-number index in the range 1.5–2 and cutoff at a few hundred keV, power-law time lags versus Fourier frequency with index 0.8, and an increase of the rms amplitude of variability and a narrowing of the autocorrelation function with increasing photon energy as they have been observed in Cygnus X-1. The spectrum at long wavelengths (radio, infrared, optical) is modeled to come from synchrotron radiation of the energetic electrons in the jet. We find flat to inverted radio spectra that extend from the radio up to about the optical band. For magnetic field strengths of the order 10⁵–10⁶ G at the base of the jet, the calculated spectra agree well in slope and flux with the observations.     

New multifrequency measurements of the spectrum of the cosmic background radiation

New measurements of the Cosmic Background Radiation temperature at 12 cm, 6.3 cm, 3 cm, 0.9 cm and 0.3 cm have made in July 1982 from the White Mountain High Altitude Research Station. The results are presented and the existence of spectral distortions discussed.     

Modeling the broadband persistent emission of magnetars

In this paper, we discuss our first attempts to model the broadband persistent emission of magnetars within a self-consistent, physical scenario. We present the predictions of a synthetic model that we calculated with a new Monte Carlo 3D radiative code. The basic idea is that soft thermal photons (e.g. emitted by the star surface) can experience resonant cyclotron upscattering by a population of relativistic electrons treated in the twisted magnetosphere. Our code is specifically tailored to work in the ultra-magnetized regime; polarization and QED effects are consistently accounted for, as well different configurations for the magnetosphere. We discuss the predicted spectral properties in the 0.1–1000 keV range, the polarization properties, and we present the model application to a sample of magnetars soft X-ray spectra.     

The beaming of external Compton emission

We consider a relativistically moving blob consisting of an isotropic electron distribution that Compton-scatters photons from an external isotropic radiation field. We compute the resulting beaming pattern, i.e. the distribution of the scattered photons, in the blob frame as well as in the observer’s frame by using the full Klein–Nishina cross section and the exact incident photon distribution. In the Thomson regime the comparison of our approach with Dermer (1995) results in concurrent characteristics but different absolute number of the scattered photons by a factor of f_corr = 3.09. Additionally, our calculation yields a slightly lower boost factor which varies the more from the corresponding value in Dermer (1995) the higher the spectral index p of the electron distribution gets.     

Fast spacecraft solar radiation pressure modeling by ray tracing on graphics processing unit

A novel method is presented to evaluate on the graphics processing unit (GPU) the force and torque on a spacecraft due to solar radiation pressure. The method employs efficient ray tracing techniques, developed in the graphics rendering discipline, to resolve spacecraft self-shadowing and reflections at faster than real-time computation speed. The primary algorithmic components of the ray tracing process which contribute to the method’s computational efficiency are described. These components include two-level bounding volume hierarchy acceleration data structures, fast ray to bounding box intersection testing using the slab intersection algorithm and fast triangle intersection testing using the Möller-Trumbore algorithm. Spacecraft material optical properties are represented as a combination of Lambertian diffuse and ideal specular reflections. Both diffuse and specular ray-surface interactions are modeled. The approach is implemented using C++ and OpenCL and executed on a consumer grade GPU. Model validation is presented comparing ray traced force and torque values to the same quantities produce by a faceted analytic model. Numerical results illustrate the impact of self-shadowing on the force and torque calculation, and demonstrate the fast computational speed that is enabled with this implementation.     

模式识别中幂变换正态性的研究

在基于模板匹配的模式识别中,当数据呈正态分布时得到的识别效果最优。幂变换是一种将非正态分布转换为正态分布的一种有效方法,文中对幂变换技术的正态性问题进行了相关的研究,并探讨了典型分布条件下的幂变换最佳取值问题,为幂变换的应用提供了一定的理论基础。     

基于复摆模型的多脉冲冲量耦合系数测量方法

在单脉冲冲量测量方法的基础上,增加激光脉冲提取和摆杆控制单元,提出了一种基于复摆模型的多脉冲冲量耦合系数测量方法。分析了多脉冲的两种测量模式及实现流程,解决了数据处理面临的新问题,并对该方法进行了检验,结果表明:所设计的激光脉冲提取和摆杆控制单元满足25Hz频率要求,可实现在40ms内提取多脉冲序列的任意一个脉冲;模拟多脉冲序列下测得两种模式15°锥形喷管的冲量耦合系数为371.0～375.3N/MW,具有很好的一致性。该方法可用于吸气式激光推进的多脉冲性能研究,并作为其他多脉冲研究方法的有效补充。     

结合不确定度的发动机模型辨识气路诊断

针对航空发动机气路诊断中测量参数个数小于待诊断参数个数的不适定问题,利用了发动机平衡技术,结合非线性的发动机数学模型,并综合考虑了测量参数的不确定度和理论模型部件性能的不确定度,建立了一种结合不确定度的发动机气路故障诊断辨识算法——变分加权最小二乘法,并将该算法应用于某发动机的诊断分析中.结果表明:运用该方法可分析出测量数据和模型计算数据之间的差别,同时,利用所得的故障参数修正量修正原发动机数学模型,使模型计算推力与试验测量推力最大偏差由8.25%减小到1.66%,耗油率最大偏差由6.25%减小到1.50%.      

基于确定学习理论的轴流压气机系统分岔预测

针对轴流压气机系统中的分岔预测问题,基于简化的Moore-Greitzer 3阶压气机模型,分析了该系统中存在的分岔现象;利用最新发展的确定学习理论,对压气机系统随着γ参数变化出现的几种典型模态的相关系统动态进行辨识,并将所学知识保存成常值RBF神经网络以构成模式库;利用该模式库构建1组嵌入了常值RBF神经网络的动态估计器;将测试模式与估计器相比,得到1组残差,并利用动态模式识别方法的残差最小原则实现了对Pitchfork分岔的预测。