我国通用航空应急管理体系构建

低空空域开放是助力我国通用航空迅速发展的重大战略性举措,同时将对通用航空在作业过程中的应急管理带来挑战。文章给出通用航空突发事件的定义,对引起通用航空突发事件的致灾因素从通用航空器、通用航空作业环境、通用航空服务保障情况做一分析。阐述了通用航空应急管理的定义。最后提出了基于应急管理平台的通用航空应急管理体系。     

风洞模型-支撑系统涡激振动测量与分析

以0.55m×0.4m低湍流航空声学风洞某模型及其支撑系统为研究对象,采用基于加速度传感器直接测量支撑系统和热线间接测量模型尾流相结合的方法,测量并分析了风洞模型-支撑系统的涡激振动模态,给出了测量方案和数据处理方法。采用基于加速度传感器的功率谱分析方法,获得了模型-支撑系统的三阶振动频率分别为31.1、120.9和221.4Hz;采用基于加速度传感器的频域滤波和频域积分方法,提高了有效信号的信噪比,获得了模型-支撑系统振动的振型和振动节点位置;采用热线测量模型尾流分离涡脱落频率的方法,获得了模型一阶和二阶振动的尾流涡激频率分别为31.1和124.1 Hz,并从测量尾流速度脉动量获得了模型振幅变化和抖振边界信息。实验结果表明,采用热线测量模型尾流从而分析模型振动的方法,有利于小尺度的模型振动测量,而且相对于加速度传感器装于模型表面的直接测量方法而言,对试验模型的绕流流场干扰较小,为测量风洞试验模型的涡激振动模态提供了一种方法。     

低速轴流压气机转子尾迹三维动态测量

对一台低速轴流压气机的转子尾迹进行了三维动态测量,采用锁相平均、方均根和功率谱密度等分析方法对低速轴流压气机转子在节流过程中尾迹流场的稳态和动态特征进行了研究.结果显示:在绝对坐标系下,转子尾迹有高总压和高方均根特征,且在不同叶高的强度不同;转子尾迹与主流的掺混作用导致平均总压升系数的快速衰减;功率谱密度分析表明,在接近失速点时,转子尾迹90%叶高以上出现0.5倍叶片通过频率的特征频带且其功率随着流量减小而增大.      

New trade tree for manned mars missions

Recent studies on human missions to Mars suggest revisiting the parameters that have the most important impact on the complexity, the initial mass in low Earth orbit, the risks and the development costs for the first journey to the red planet. In the last NASA reference mission, a trade tree is proposed.     

United Nations Human Space Technology Initiative (HSTI)

The Human Space Technology Initiative was launched in 2010 within the framework of the United Nations Programme on Space Applications implemented by the Office for Outer Space Affairs of the United Nations. It aims to involve more countries in activities related to human spaceflight and space exploration and to increase the benefits from the outcome of such activities through international cooperation, to make space exploration a truly international effort.     

A hybrid attitude controller consisting of electromagnetic torque rods and an active fluid ring

In this paper, a novel hybrid actuation system for satellite attitude stabilization is proposed along with its feasibility analysis. The system considered consists of two magnetic torque rods and one fluid ring to produce the control torque required in the direction in which magnetic torque rods cannot produce torque. A mathematical model of the system dynamics is derived first. Then a controller is developed to stabilize the attitude angles of a satellite equipped with the abovementioned set of actuators. The effect of failure of the fluid ring or a magnetic torque rod is examined as well. It is noted that the case of failure of the magnetic torque rod whose torque is along the pitch axis is the most critical, since the coupling between the roll or yaw motion and the pitch motion is quite weak. The simulation results show that the control system proposed is quite fault tolerant.     

翼型前缘变形对动态失速效应影响的数值计算

翼型或机翼的动态失速效应所引起的低头力矩和正气动阻尼限制了飞行器气动性能的提高,甚至可能诱导发生不稳定运动。应用于小尺寸机翼的前缘动态变形（DDLE）技术,通过实时改变前缘形状,能够改善翼型前缘区域的速度梯度,进而抑制动态失速效应。采用转捩剪切应力输运（SST）黏性模型结合分区混合动态网格技术,研究了这种前缘变形对机翼俯仰运动所引起的非定常流动的影响,得到通过小幅度前缘变形抑制和延迟动态失速的方法,从而提高翼型的气动性能。翼型NAC A0012的数值模拟结果与动态失速风洞试验结果比较表明：所使用的数值计算方法能够较为准确地模拟翼型在动态失速过程中升力系数与俯仰力矩系数的变化情况,可用于研究前缘变形对翼型俯仰运动所引起的非定常流动的影响。前缘动态变形翼型俯仰运动过程的非定常流场的数值模拟表明：在大迎角下不同幅度的前缘下垂运动能够抑制流动分离的发生,从而抑制动态失速,但在大迎角下小幅度高频率的前缘下垂变形能更高效地抑制动态失速;前缘变形幅度以及变形沿中弧线的分布对升力系数和俯仰力矩系数的影响并不明显。     

双后掠鸭翼气动特性的数值模拟

首先针对具有中等前缘后掠角梯形鸭翼的缺点提出双后掠鸭翼概念,然后分别对安装梯形鸭翼和双后掠鸭翼的近距耦合鸭式布局的气动性能进行数值模拟研究,分析影响双后掠鸭翼气动性能的流动机理。研究表明：在大迎角时,对于双后掠鸭翼,具有较大前缘后掠角的外翼段可以使鸭翼涡在涡核破裂后仍能形成稳定集中涡并保持较高的强度,增加鸭翼本身的失速迎角,并通过诱导作用改善机翼外翼段流场,进而提高全机大迎角性能,但在小迎角时会破坏鸭翼附着流或前缘气泡涡的发展,造成略微的升力损失。拥有较大失速迎角的双后掠鸭翼在小迎角时具有较大的可用偏度,可以增强布局的抬头控制能力。双后掠鸭翼在满足隐身约束的前提下,超声速阻力较小,具有较好的超声速性能。     

基于三维最小二乘方法的空间直线度误差评定

空间直线度误差是评定机械产品精度的一项重要指标,实际工程中对空间直线度误差评定算法的精度要求越来越高.为了准确评定空间直线度误差,参照国家标准(GB/T 11336—2004),采用三维最小二乘方法建立了空间直线拟合的数学模型,并给出了该数学模型的精确解.基于最小二乘拟合中线,采用空间投影、坐标变换和格点法求得最小二乘中线包容圆柱面直径.采用数值算例验证了新方法的有效性.提出的空间直线度误差评定方法精度高、鲁棒性好且易于编程实现.     

Strong geomagnetic activity forecast by neural networks under dominant southern orientation of the interplanetary magnetic field

The paper deals with the relation of the southern orientation of the north–south component _Bz$B_z$ of the interplanetary magnetic field to geomagnetic activity (GA) and subsequently a method is suggested of using the found facts to forecast potentially dangerous high GA. We have found that on a day with very high GA hourly averages of _Bz$B_z$ with a negative sign occur at least 16 times in typical cases. Since it is very difficult to estimate the orientation of _Bz$B_z$ in the immediate vicinity of the Earth one day or even a few days in advance, we have suggested using a neural-network model, which assumes the worse of the possibilities to forecast the danger of high GA – the dominant southern orientation of the interplanetary magnetic field. The input quantities of the proposed model were information about X-ray flares, type II and IV radio bursts as well as information about coronal mass ejections (CME). In comparing the GA forecasts with observations, we obtain values of the Hanssen–Kuiper skill score ranging from 0.463 to 0.727, which are usual values for similar forecasts of space weather. The proposed model provides forecasts of potentially dangerous high geomagnetic activity should the interplanetary CME (ICME), the originator of geomagnetic storms, hit the Earth under the most unfavorable configuration of cosmic magnetic fields. We cannot know in advance whether the unfavorable configuration is going to occur or not; we just know that it will occur with the probability of 31%.