软件技术专业“订单式”人才培养模式的探索和实践

本文从"订单式"人才培养模式的客观需求人手,依据课题的研究和实践经验,综述了软件技术专业"订单式"人才培养的开展过程,分析了"订单式"人才培养模式的关键问题并提出了解决方案.     

外弹道测量数据采集与处理技术

数据采集与处理技术是数据处理的关键。主要介绍外测事后数据处理过程中测量数据采集、异常数据识别、数据中奇异项剔除、数据丢点、重点检测方法、数据取齐、加密、压缩与采样时间校正、数据平滑滤波等关键技术,其对于研究数据处理新方法和提高数据处理精度,具有一定的参考价值。     

定向凝固时热溶质对流对Al/AlLi共晶生长形态稳定性的影响

在垂直向上定向凝固条件下,研究了热溶质对流对二元亚共晶 Al-Li合金 Al/ Al Li共晶生长形态稳定性的影响。结果表明,晶体生长初期,热溶质对流较微弱,对界面形态稳定性无明显的影响,晶体以完全的Al/ Al Li共晶方式生长。当热溶质对流较强烈时,对界面形态稳定性产生严重的影响。平面界面失稳破开时,单相胞状晶领先生长。在单相胞状晶之间以 Al/ Al Li共晶方式生长。获得了二元亚共晶 Al-Li合金共晶的稳定性生长条件。     

A Cosmic Microscope to Probe the Universe from Present to Cosmic Dawn:Dual-element Lowfrequency Space VLBI Observatory

A space-based Very Long Baseline Interferometry (VLBI) program, named as the Cosmic Microscope, is proposed to involve dual VLBI telescopes in the space working together with giant ground-based telescopes (e.g., Square Kilometre Array, FAST, Arecibo) to image the low radio frequency Universe with the purpose of unraveling the compact structure of cosmic constituents including supermassive black holes and binaries, pulsars, astronomical masers and the underlying source, and exoplanets amongst others. The operational frequency bands are 30, 74, 330 and 1670 MHz, supporting broad science areas. The mission plans to launch two 30-m-diameter radio telescopes into 2 000 km×90 000 km elliptical orbits. The two telescopes can work in flexibly diverse modes. (i) Space-ground VLBI. The maximum space-ground baseline length is about 100 000 km; it provides a high-dynamic-range imaging capacity with unprecedented high resolutions at low frequencies (0.3 mas at 1.67 GHz and 20 mas at 30 MHz) enabling studies of exoplanets and supermassive black hole binaries (which emit nanoHz gravitational waves). (ii) Space-space single-baseline VLBI. This unique baseline enables the detection of flaring hydroxyl masers, and more precise position measurement of pulsars and radio transients at mas level. (iii) Single dish mode, where each telescope can be used to monitor transient bursts and rapidly trigger follow-up VLBI observations. The large space telescope will also contribute in measuring and constraining the total angular power spectrum from the Epoch of Reionization. In short, the Cosmic Microscope offers astronomers the opportunity to conduct novel, frontier science.      

Feasibility study of creep feed grinding of 300M steel with zirconium corundum wheel

The ultrahigh strength 300M steel has been commonly used in the manufacture of aircraft landing gear and rotor shaft parts due to its excellent mechanical properties. Creep feed grinding is one of the essential operations during the whole component manufacturing processes. In this work, the feasibility of creep feed grinding of 300M steel by using the hard zirconium corundum wheel was theoretically and experimentally evaluated. A variety of responses including grinding forces, temperature fields...     

蜂窝芯体材料面外等效弹性模量预测与分析

基于最小势能原理和最小余能原理,选择比Kelsey模型所用表征单元更简化的单元为研究对象,推导出与之完全相同的蜂窝芯体面外等效弹性模量的解析表达式。采用有限元法预测一组典型商用正六边形蜂窝芯体的面外等效弹性模量,并将解析解模型预测值、有限元模型预测值与厂家公布的材料试验数据进行对比。提出一组基于解析解模型的修正公式用于预测与分析典型正六边形蜂窝芯体的面外等效弹性模量。     

基于立体观测的空间目标天基光学监视定位

利用天基观测平台实现对空间目标的有效监视是空间监视的发展方向和必然趋势。本文提出充分利用天基光学观测灵活性,采用基于双／多星立体观测定位的方法,提高空间目标监视定位效能,并就系统观测条件进行分析。     

跟踪传感器空域覆盖性能分析

针对天基光学跟踪传感器覆盖问题,将点覆盖数值仿真模型扩展到空域,提出了一种基于视函数的跟踪传感器覆盖计算方法.在典型圆轨道星座下,对所提方法进行数值仿真,并分析了覆盖性能的影响因素,为天基光学低轨星座设计和跟踪传感器管理调度提供重要的参考和支持.     

重构飞行控制技术研究综述

重构飞行控制技术的研究源于保障飞行安全性的考虑,即在故障发生的情况下,通过对飞行控制系统进行重构,提高飞行的安全性和可靠性.在空中交通日益繁忙的今天,对飞行的安全性和可靠性提出了更高的要求,因而重构飞行控制技术具有重要的研究价值.国内外就重构飞行控制技术展开了一系列的研究计划,通过这些研究计划,可以了解重构飞行控制技术发展的过程和研究现状,结合最新的研究进展总结了目前的研究方向和热点问题,明确了今后该领域的研究方向和重点.     

飞机尾涡对飞行安全的影响

针对一次夜间双机编队飞行时发生的空中相撞事故,根据机载黑匣子记录的飞机飞行参数,判明机进入了长机尾涡,利用记录的飞行参数,阐明了飞机进入尾涡的征兆,以及尾涡对飞机仪表,动态和操纵的影响,找出了飞机发生相撞的原因,为防止类惟事故发生,提出了僚机进入长机尾涡后应采取的措施,以供飞行行人员参考。