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。     

温度参数下轴编C/C复合材料的超高温热结构性能分析

为了研究轴编碳/碳（C/C）复合材料的超高温热结构性能,开展了2800℃超高温载荷下复合材料的拉伸实验,表征了复合材料组分材料的高温失效形貌;提出了立方体单胞和正六棱柱单胞的温度周期性边界条件的算法和预测复合材料等效热结构参数的方法,在材料属性各向同性正六棱柱单胞模型上验证了方法的正确性;最后建立了轴编C/C复合材料的代表性体积单元,计算了复合材料随温度载荷变化下的等效热结构参数,与实验数据进行了对比分析。分析表明：开展的轴编C/C复合材料的超高温拉伸实验,可以得到复合材料在2800℃载荷下复合材料的等效刚度值,同时分析了轴向试件和径向试件的高温失效机理,径向试件的纤维束拉伸强度对复合材料的径向拉伸强度起到决定性的作用。在应用位移以及温度周期性边界条件的基础上,提出的方法可以得到随温度载荷变化下复合材料的等效热结构参数,得出复合材料在横向满足近似各向同性的特性,预测结果表明只改变温度参数下复合材料的等效热导率不会发生改变。提出的方法同样也适用于其他编织复合材料的热结构性能研究。     

叶栅绕流计算的高分辨率隐式解法

以一种性能优越的高分辨率格式为基础, 发展了其隐式解法, 提出并实现了与这种格式相适应的隐式边界处理过程, 从而显着提高了高分辨率格式的收敛速度。用不同来流条件下叶栅绕流数组计算结果与实验做了对比, 以说明解的准确程度和本文算法的效果。