基于TMS320C80的BP算法并行实现的研究

结合 TMS32 0 C80的编程结构 ,利用神经网络的权并行性和神经元并行性 ,提出了BP算法的并行实现方法 ,并解决了存储器访问冲突、数据双缓冲传输、PP细粒度并行和死锁等问题。结果表明 ,该并行 BP算法十分有效。     

基于并行禁忌遗传算法(PTGA)的预警卫星传感器调度研究

对预警卫星的传感器调度进行了研究，提出了传感器管理调度的系统组成。通过对传感器调度的分析，建立起相应的数学模型，定义了评价指标。结合并行遗传算法和禁忌搜索的特点，提出了一种新的解决预警卫星传感器调度问题的并行禁忌遗传算法(PTGA)。该算法采用多种群和禁忌搜索思想改进遗传算法的性能，从而提高整个算法的收敛速度和精度。实验结果表明该算法有效地解决了多目标情况下的传感器实时调度问题，并优于一般启发式算法。     

轴对称横向喷流强干扰流场的巨型机向量并行计算

本文在国产巨型计算机ＹＨ－１和ＹＨ－２上对ＭａｃＣｏｒｍａｃｋ显格式解轴对称横向喷流强干扰流场的计算程序进行了重构和向量优化使其能并行执行。得到该程序在ＹＨ－１上的向量加速比约为６．０，ＹＨ－２单机向量运行速度约为ＹＨ－１上的向量运行速度的３倍。与传统的串行计算相比较，并行计算大大缩短了程序运行的ＣＰＵ时间。     

空间光学精密展开机构展开方法的初步探讨

文章对空间光学精密展开机构(以下简称展开机构)进行分类,分析了几种典型可展开空间光学系统的展开方法和特点。讨论了展开机构设计需要考虑的主要因素,并给出设计建议。     

大型转动机械碰摩故障分析的声发射检测系统

汽轮发电机、空气压缩机等采用油膜支撑的大型转动机械,由于安装或运行中的原因,在转子旋转过程中,可能和器壁发生轻微的摩擦和碰击,简称碰摩.声发射技术在碰摩发生特别是故障早期诊断上有优越性.本系统的特点是没有沿用传统的计数、幅度、能量和持续时间等声发射特性参数,而是在声发射包络信号的频率分析中进行特征提取.声发射发生的过程分析和现场试验都表明这种方法对碰摩检测很敏感,在碰摩发生的起始阶段,包络谱中与转速同步的周期性分量显著增加.根据这种新的设计思想自行研制了BUAA碰摩声发射检测仪并对此作了介绍.     

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.     

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.     

基于6SPS并联机构标定新方法

系统研究6SPS并联机构标定的方法。研究中应用激光跟踪仪测量、基于并联机构正解和定位误差旋量的计算,正交试验进行试验设计,应用非线性最小二乘参数辨识。仿真验证辨识的几何误差可以等于假定值,试验验证位姿精度提高了10倍。     

配对进近模式分析及研究进展

配对进近模式是在近距平行跑道上运行的,旨在提高仪表气象条件下的进场效率的一种高效进近模 式,该模式的完整流程在国内鲜有阐述。本文重点分析配对进近程序在近距平行跑道上运行时各阶段的流程, 以及配对进近程序的实施对机型、设备以及人员的具体要求;结合目前国内近距平行跑道的运行情况,国际上 对配对进近模式的研究和应用现状,指出我国引进配对进近模式的迫切性以及该模式今后的研究和发展趋势。