基于高速慢车的航空发动机快速响应控制

针对传统航空发动机响应速度慢,难以在紧急事件中用于控制受损飞机完成起降过程的问题,采用高速慢车控制模式来提升发动机加速性能,通过增加发动机在慢车时高压压气机转速,为加速前期提供更大的燃油流量,从而缩短发动机从慢车至最大状态的加速时间。为保证慢车时高压转子转速提高的同时发动机推力和稳定裕度不变,通过修改高压压气机可调导叶控制计划来调整高压转子工作点。仿真结果显示,与原有控制相比,采用高速慢车快速响应控制模式的发动机加速上升时间从原来的2.00s缩短至1.86s,而高压压气机最小喘振裕度仅由16.01%下降至14.81%,同时慢车推力基本保持不变。     

无人直升机悬停低速段的不确定性仿真验证

在无人直升机控制律的设计过程中,需要对无人直升机进行建模,并对飞行中产生的一些不确定性因素进行仿真验证.目前,很多不确定性因素的描述是在非线性的环境中加入一些简单的扰动,然而能够确切地描述无人直升机动态特性的非线性模型在MATLAB中很难搭建.为此,文章从工程研究的角度,提出了在无人直升机线性模型组的基础上进行不确定性仿真验证的方法,从物理特性的角度描述无人直升机在悬停低速飞行时的对象特性不确定性,选择不确定或扰动因子;在MATLAB中建立了仿真模型,进行了无人直升机悬停低速段不确定性的验证.此方法简单、快速,并且能正确地反应无人直升机悬停低速段的不确定性,具有一定的工程意义.     

飞行控制技术面临的挑战与发展

总结了飞行器的发展趋势,明确了飞行控制领域的前沿问题与挑战,概括了飞行控制技术的基础问题和关键技术,分析了现阶段飞行控制技术研究进展,对未来飞行控制技术的发展提出了建议与思考。     

卫星控制中心系统平台的高可用设计与实现

卫星控制中心是卫星地面测控管理系统的重要组成部分。随着信息技术的飞速发展和测控关键业务量的增长,高可用性、高可靠性及易维护日益成为卫星控制中心系统的设计目标。为满足卫星测控任务的需求,本文描述了卫星控制中心的网络系统、数据处理系统和数据库集群系统的高可用设计,并给出具体项目的成功实现。     

Evolution of the orbital elements for objects with high area-to-mass ratios in geostationary transfer orbits

A new population of uncatalogued objects in geosynchronous Earth orbits (GEO), with a mean motion of about 1 rev/day and eccentricities up to 0.6, has been identified recently. The first observations of this new type of objects were acquired in the framework of the European Space Agency’s (ESA) search for space debris in GEO and the geostationary transfer orbit (GTO) using the ESA 1-m telescope on Tenerife. Earlier studies have postulated that the perturbations due to the solar radiation pressure can lead to such large eccentricities for GEO objects with a high area-to-mass ratio (A/M). The simulations showed that the eccentricities of GEO objects with large A/M exhibit periodic variations with periods of about one year and amplitudes depending on the value of A/M. The findings of these studies could be confirmed by observations from the ESA 1-m telescope on Tenerife.     

Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

Cosmic ray studies at Moussala – Past,present and future

We review the main activities carried out at Moussala peak (2925 m above sea level, 42°11′N, 23°35′E) station in Bulgaria, connected with cosmic ray investigations during the last five decades. Several important results obtained at the station are reported. The detector design and corresponding methodological studies of the presently operational devices are shown as well, precisely the Cherenkov light telescope, lead free neutron monitor and muon telescope. The scientific potential of the existing complex is discussed.     

Investigation of natural and artificial stimulation of the ionospheric Alfvén resonator at high latitude

A brief review is provided of recent progress in understanding the ionospheric Alfvén resonator (IAR) at high latitude. Firstly, naturally occurring resonances of the IAR as detected by pulsation magnetometers in the auroral zone at Sodankylä and in the polar cap at Barentsburg are considered. The characteristics of the IAR in the two regions are broadly similar, although the effects of solar illumination are less clear at the higher latitudes. Secondly we review recent attempts to stimulate the IAR through high-power radio frequency experiments both in the auroral zone at Tromsø with the European Incoherent SCATter (EISCAT) heater, and within the polar cap at Longyearbyen with the Space Plasma Exploration by Active Radar (SPEAR) facility. In the auroral zone at, Tromsø the stimulated IAR has been observed by ground-based magnetometers, and through electron acceleration observed on the FAST spacecraft. At SPEAR in the polar cap, the stimulated IAR has been investigated, with ground magnetometers, with the first results indicative of a positive detection.     

长配管、高落差空调系统的计算机仿真与试验研究

空调系统在长配管、高落差情况下其运行性能和可靠性会受到影响。建立数学模型预测长配管、高落差空调系统的性能，可以提供给用户准确的性能资料，指导用户合理安装空调器，提高产品的可靠性。     

凝胶点官能度是重均官能度,还是数均官能度

Flory和Stockmayer等的凝胶化理论用重均官能度表示凝胶点或凝胶生成的临界条件,虽已有50多年的历史,并为各国学者所公认,但从分析凝胶点定义的物理意义出发,只要用简单的数学分析,即可证明用重均官能度而不用数均官能度表示凝胶点,与反应程度定义的物理意义和Flory的两个基本假设不符。凝胶化理论新概念用数均官能度表示凝胶点,则不存在不符的问题。