以相对偏差平方和为指标函数的最小二乘法

就测量中最小二乘法用于静态模型估计的问题,分析了传统最小二乘法在某些实验条件下应用的不合理现象,提出以相对偏差平方和为指标函数的最小二乘法。简记LSR法。给出了该方法的实用公式,分析了数学特征并证明在所给实验条件下具有无偏性、一致性,有效性.给出了用该方法拟合电位差计静态特性方程的例子。证明该方法在测量工作中是有实际意义的。     

Evaluation of airborne data link communication

An experimental prototype of a cockpit data link communication interface (modified Navigation Display (ND) and Multi-purpose Control and Display Unit (MCDU)) was developed and tested in an Airbus A340 Full Flight Simulator. 8 crews (16 professional pilots) performed simulator flights in a mixed voice and data link scenario. After each experiment video recordings were presented to the pilots and they were asked to estimate subjective strain (NASA task load index) and situational aspects retrospectively. Results show an increase in subjective strain and a decrease of ‘feeling of sovereignty’ and situation awareness under data link conditions. The effect is similar to the one caused by higher workload.     

航空发动机寿命延长控制综述

传统航空发动机控制系统设计,只关注发动机性能,而寿命延长控制(Life Extending Control,LEC)将发动机寿命纳入到发动机控制系统设计要求中,以期在控制系统中解决寿命问题.在总结国外相关文献的基础上,简要回顾了航空发动机寿命延长控制的研究背景和价值;详细阐述了发动机寿命延长控制实现策略及其关键技术;并对航空发动机寿命延长控制结构进行介绍,提出多级延寿控制系统结构以解决控制器冲突问题;结合国内状况,针对发动机寿命延长控制技术给出一些建议.     

The case for massive,evolving winds in black hole X-ray binaries

In the last decade, high-resolution X-ray spectroscopy has revolutionized our understanding of the role of accretion disk winds in black hole X-ray binaries. Here I present a brief review of the state of wind studies in black hole X-ray binaries, focusing on recent arguments that disk winds are not only extremely massive, but also highly variable. I show how new and archival observations at high timing and spectral resolution continue to highlight the intricate links between the inner accretion flow, relativistic jets, and accretion disk winds. Finally, I discuss methods to infer the driving mechanisms of observed disk winds and their implications for connections between mass accretion and ejection processes.     

一种正交跳频信号动态分选方法

针对复杂电磁环境下正交跳频信号分选时效不高问题,提出了一种正交跳频信号动态分选方法。首先基于滑动窗口的数据流模型,采用构造型神经网络对跳频信号频域数据和方位信息动态聚类,减轻噪声等因素影响,解决方位信息和幅度关联模糊性的问题;再在相应的覆盖簇内运用时频关联方法,实现正交跳频信号的动态分选,实验结果表明该方法是有效的。
     

推进剂贮箱锥柱形金属膜片的翻转特性研究

基于MSC.Marc非线性有限元软件,对推进剂贮箱锥柱形金属膜片的变形进行仿真研究。模拟了膜片的翻转变形过程,分析了膜片翻转变形规律和失效因素,提出了膜片有效稳定翻转的条件。     

Late stages of stellar evolution – Herschel’s contributions

Cool objects glow in the infrared. The gas and solid-state species that escape the stellar gravitational attraction of evolved late-type stars in the form of a stellar wind are cool, with temperatures typically ?1500 K, and can be ideally studied in the infrared. These stellar winds create huge extended circumstellar envelopes with extents approaching 10¹⁹${10}^{19}$ cm. In these envelopes, a complex kinematical, thermodynamical and chemical interplay determines the global and local structural parameters. Unraveling the wind acceleration mechanisms and deriving the complicated structure of the envelopes is important to understand the late stages of evolution of ∼97% of stars in galaxies as our own Milky Way. That way, we can also assess the significant chemical enrichment of the interstellar medium by the mass loss of these evolved stars. The Herschel Space Observatory is uniquely placed to study evolved stars thanks to the excellent capabilities of the three infrared and sub-millimeter instruments on board: PACS, SPIRE and HIFI. In this review, I give an overview of a few important results obtained during the first two years of Herschel observations in the field of evolved low and intermediate mass stars, and I will show how the Herschel observations can solve some historical questions on these late stages of stellar evolution, but also add some new ones.     

基于B/S结构虚拟仪器系统设计与实现

在网络技术高速发展的基础上,针对频谱分析仪的共享操作以及远程操作等问题,提出基于B/S（浏览器/服务器）结构的网络虚拟仪器系统的解决方案。系统通过仪器控制软件完成对多种接口频谱仪的监视与控制,并通过服务端软件以页面形式实现系统与用户的交互。该系统可以部署在局域网或者互联网上,用户可以通过浏览器实现对频谱分析仪的访问与操作。根据方案开发的实验系统,通过测试已经具备了设计的功能需求,实现了频谱仪的网络共享和远程操作,为用户提供了一种方便、容易的仪器操作方式,具有一定实际应用价值。