面向单机相依任务调度的GPU并行蚁群算法

蚁群算法是一种具有高度并行特征的群智能算法,串行实现过程中具有收敛速度慢的特点,在将其应用到相依任务序列的单机调度问题中时,以任务在不同作业序下的完成时间为基础,建立了单机调度问题的TSP模型。以任务完成时间最优化为目的,实现了一种求解相依任务单机调度的改进蚁群算法,并基于GPU对其进行了并行化设计。实验表明该算法能够完成相依任务的调度处理,通过并行化得到了较高的加速比。     

关于飞机数字化定义体系的研究

飞机产品的数字化定义体系由多个部分组成。各部分之间必须协调发展,按照一个统一的目标建立起一个互相支撑、互相关联的有机体系。国外先进的航空制造企业已经建立了比较完整的数字化定义体系。国内的航空企业还基本处于单项技术的研究、应用阶段。     

压气机静子叶片转角主备控制器转换装置改进

为了确保某型航空发动机高压压气机可调静子叶片转角控制系统主备控制器转换的可靠性,对系统原有的控制器转换装置进行了改进,加入了新的转换机构.仿真计算结果表明,若数字电子控制器故障后,未按照预定要求输出0脉冲占空比,而输出了固定的非0脉冲占空比信号或随机的不可预测的脉冲占空比信号,原系统的正常工作将受到较严重的影响;而采用...     

基于Mori-Tanaka有限元法的粘弹复合推进剂非线性界面脱粘

为了研究复合推进剂基体的大应变粘弹性和界面的非线性脱粘,将Mori-Tanaka法和有限元数值求解相结合,提出了一种Mori-Tanaka有限元法。同时,为验证该方法的有效性,针对推进剂夹杂随机填充的特点,提出了一种含非线性界面脱粘的数值仿真法。最后以某推进剂配方为算例,对两种方法的计算结果了进行比较。结果表明,两种方法结果接近,从而验证了Mori-Tanaka有限元法的有效性,且该方法计算量小,极大的提高了计算效率。两种方法的提出,可以有效的用来分析界面对推进剂力学性能的影响。     

Near Infrared Spectrometer for the Near Earth Asteroid Rendezvous Mission

The Near-Infrared Spectrometer (NIS) instrument on the Near-Earth Asteroid Rendezvous (NEAR) spacecraft is designed to map spectral properties of the mission target, the S-type asteroid 433 Eros, at near-infrared wavelengths diagnostic of the composition of minerals forming S asteroids. NIS is a grating spectrometer, in which light is directed by a dichroic beam-splitter onto a 32-element Ge detector (center wavelengths, 816–1486 nm) and a 32-element InGaAs detector (center wavelengths, 1371–2708 nm). Each detector reports a 32-channel spectrum at 12-bit quantization. The field-of-view is selectable using slits with dimensions calibrated at 0.37° × 0.76° (narrow slit) and 0.74° × 0.76° (wide slit). A shutter can be closed for dark current measurements. For the Ge detector, there is an option to command a 10x boost in gain. A scan mirror rotates the field-of-view over a 140° range, and a diffuse gold radiance calibration target is viewable at the sunward edge of the field of regard. Spectra are measured once per second, and up to 16 can be summed onboard. Hyperspectral image cubes are built up by a combination of down-track spacecraft motion and cross-track scanning of the mirror. Instrument software allows execution of data acquisition macros, which include selection of the slit width, number of spectra to sum, gain, mirror scanning, and an option to interleave dark spectra with the shutter closed among asteroid observations. The instrument was extensively characterized by on-ground calibration, and a comprehensive program of in-flight calibration was begun shortly after launch. NIS observations of Eros will largely be coordinated with multicolor imaging from the Multispectral Imager (MSI). NIS will begin observing Eros during approach to the asteroid, and the instrument will map Eros at successively higher spatial resolutions as NEAR's orbit around Eros is lowered incrementally to 25 km altitude. Ultimate products of the investigation will include composition maps of the entire illuminated surface of Eros at spatial resolutions as high as 300 m.     

Energetic Particles Investigation (EPI)

The Energetic Particles Investigation (EPI) instrument operates during the pre-entry phase of the Galileo Probe. The major science objective is to study the energetic particle population in the innermost regions of the Jovian magnetosphere — within 4 radii of the cloud tops — and into the upper atmosphere. To achieve these objectives the EPI instrument will make omnidirectional measurements of four different particle species — electrons, protons, alpha-particles, and heavy ions (Z > 2). Intensity profiles with a spatial resolution of about 0.02 Jupiter radii will be recorded. Three different energy range channels are allocated to both electrons and protons to provide a rough estimate of the spectral index of the energy spectra. In addition to the omnidirectional measurements, sectored data will be obtained for certain energy range electrons, protons, and alpha-particles to determine directional anisotropies and particle pitch angle distributions. The detector assembly is a two-element telescope using totally depleted, circular silicon surfacebarrier detectors surrounded by a cylindrical tungsten shielding with a wall thickness of 4.86 g cm^-2. The telescope axis is oriented normal to the spherical surface of the Probe's rear heat shield which is needed for heat protection of the scientific payload during the Probe's entry into the Jovian atmosphere. The material thickness of the heat shield determines the lower energy threshold of the particle species investigated during the Probe's pre-entry phase. The EPI instrument is combined with the Lightning and Radio Emission Detector (LRD) such that the EPI sensor is connected to the LRD/EPI electronic box. In this way, both instruments together only have one interface of the Probe's power, command, and data unit.     

Improved strapdown coning algorithms

Three improved algorithms for strapdown attitude computation utilizing accumulated gyro increments from the previous and current update are developed and evaluated analytically under classical coning motion. The error criterion of Miller is derived directly from the rotation vector concept. The accuracy of updating rotation vector estimation can be improved at least two orders of magnitude as compared with those of conventional algorithms. The proposed algorithm is equivalent to increasing the number of gyro samples used in the conventional method and it requires less computer loading     

前台阶流场的传热实验研究

本文尝试用瞬态实验方法, 在卢德威格风洞实验台上, 对小台阶高度 (H=4.0mm)的前台阶二维流场进行传热实验研究, 测定了当雷诺数为 11800至32200时的流场内热流通量和努谢尔特数的变化规律以及努谢尔特数随雷诺数变化的准则关系式。实验结果是令人满意的。      

飞机风挡透明件的鸟撞分析

 本文研究了风挡透明件鸟撞动力响应的分析模型和方法。考虑了撞击载荷与风挡透明件动力响应的耦合作用和非线性效应。为了能方便地使用现有的非线性有限元分析程序并避免数值解的振荡现象,在研究中不采用常用的拉格朗日法和罚函数法,而是采用动量平衡法。同时,为了避免不断调整撞击接触点和修改网格,本文采用超弹性的橡皮材料来模拟鸟体,而不是象国外那样采用流体柱。研究和比较了衍生动载荷响应解,并提出相应的看法。