Analysis on Potential Conflict Frequency of Intersected Air Routes in Terminal Airspace Design

In order to obtain accurate conflict risks in terminal airspace design, the concept and calculation model of potential conflict frequency for intersected routes are proposed. Conflict frequency is represented by the product of horizontal conflict frequency and vertical conflict probability. The horizontal conflict frequency is derived from the probability density distribution of conflicts in a period of time. Based on the recorded radar trajectory data, the concept and model of ROUTE distance are proposed, and the probability density function of aircraft height at a specified ROUTE distance is deduced by kernel density estimation. Furthermore, vertical conflict probability and its horizontal distribution are achieved. Examples of three intersected arrival and departure route design schemes are studied. Compared with scheme 1, the conflict frequency values of the other two improved schemes decrease to 53 % and 24%, respectively. The results show that the model can quantify potential conflict frequency of intersec ted routes.     

On the large-scale structure of the tail current as measured by THEMIS

The magnetic field structure and the spatial characteristics of the large-scale currents in the magnetospheric tail were studied during quiet and moderately disturbed geomagnetic conditions in 2009. The magnetic field of the currents other than the tail current was calculated in terms of a paraboloid model of the Earth’s magnetosphere, A2000, and was subtracted from measurements. It was found on the base of obtained tail current magnetic field radial distribution that the inner edge of the tail current sheet is located in the night side magnetosphere, at distances of about 10 R_E and of about 7 R_E during quiet and disturbed periods respectively. During the disturbance of February 14, 2009 (Dst_min ∼ −35 nT), the B_x and the B_z component of the tail current magnetic field near its inner edge were about 60 nT, and −60 nT that means that strong cross-tail current have been developed. The tail current parameters at different time moments during February 14, 2009 have been estimated. Solar wind conditions during this event were consistent with those during moderate magnetic storms with minimum Dst of about −100 nT. However, the magnetospheric current systems (magnetopause and cross-tail currents) were located at larger geocentric distances than typical during the 2009 extremely quiet epoch and did not provide the expected Dst magnitude. Very small disturbance on the Earth’s surface was detected consistent with an “inflated” magnetosphere.     

基于MHSS算法的ARAIM完好性和可用性预测

传统的接收机自主完好性监视只能提供非精密进近阶段的完好性监视,无法实现对完好性要求更加严格的飞行阶段的监视,而高级接收机自主完好性监视（AdvancedReceiverAutonomousIntegrityMonitoring,ARAIM）可以在精密进近阶段为飞机提供满足航向信标性能垂直引导（LocalizerPerformancewithVerticalguidance,LPV）的完好性监视服务。文章基于多假设分组解算法,根据目前的星座环境,结合民航不同飞行阶段的应用需求,对ARAIM算法进行仿真研究。针对水平保护级（HorizontalProtectionLevel,HPL）和垂直保护级（VerticalProtectionLevel,VPL）的指标,在不同星座组合环境下,选取南北半球不同经纬度的5个观测机场,分别仿真了HPL和VPL的变化情况,并对全球HPL和VPL平均分布趋势,以及以99%的概率满足LPV-200进近可用性指标时,ARAIM可用性的全球覆盖率进行了仿真预测分析。仿真结果表明,不论是全球定位系统和格洛纳斯双星座还是增加北斗卫星导航系统后的三星座,5个观测机场的HPL和VPL均能满足LPV-200进近对完好性指标的要求;但在全球范围内,双星座条件下,ARAIM并不能完全支持LPV-200进近对完好性监视的要求,而三星座则可大大提高ARAIM的可用性,为民航用户提供满足精密进近的所需导航服务性能。     

气压垂直导航中修正高度分析

在世界海拔最高民用机场四川稻城亚丁机场的基于性能导航(PBN)飞行程序设计过程中,由于GPS在垂直方向精度较低,最后进近航段采用气压垂直导航(Baro-VNAV).但机场海拔高,这种导航方式受到修正高度的影响较大.因此通过对ISA偏差对气压高度的影响公式进行推导,得出修正高度公式,利用Matlab对机场温度、航段高、机场标高与修正高度H修的关系进行分析,并以四川稻城亚丁机场Baro-VNAV实例进行了验证.最终给出了在PBN飞行程序设计过程中的建议.     

Performance evaluation of IRI-2007 at equatorial latitudes and its Matlab version for GNSS applications

International Reference Ionosphere (IRI) model is the widely used empirical model for ionospheric predictions, especially TEC which is an important parameter for radio navigation and communication. The Fortran based IRI-2007 does not support real-time interactive visualization and debugging. Therefore, the source code is converted into Matlab and is validated for the purposes of this study. This facilitates easy representation of results and for near real-time implementation of IRI in the applications including spacecraft launching, now casting, pseudolite based navigation systems etc. In addition, the vertical delay results over the equatorial region derived from IRI and GPS data of three IGS stations namely Libreville (Garbon, Africa), Brasilia (Brazil, South America) and Hyderabad (India, Asia) are compared. As the IRI model does not account for plasmasphere TEC, the vertical delays are underestimated compared to vertical delays of GPS signals. Therefore, the model should be modified accordingly for precise TEC estimation.     

一种新型垂直起降升力装置的气动特性分析与数值仿真

飞行器的垂直起降性能具有很高的军事价值和商业价值。但是目前垂直起降升力装置存在结构复杂,耗油量大,对地面热蚀严重等诸多问题,并且还限制了飞行器原有的性能,因此研究新型高效、简单实用的垂直起降升力装置迫在眉睫。本文基于二维N-S方程组和Spalart-Allmaras湍流模型,利用Fluent流场仿真软件,研究论证了一种...     

火箭弹垂直发射动力学建模与仿真

首先建立了火箭弹垂直发射的弹道模型,然后研究了升阻比、弹道倾角等参数的变化对火箭弹射程的影响,并分别对这两种情况进行了仿真。仿真结果表明,滑翔飞行时,在一定程度上增大了升阻比,有助于增大火箭弹的射程;另外在转弯结束时,弹道倾角的变化对火箭弹射程也有一定影响。     

V形尾翼气动布局纵向力矩特性研究

针对某无人战斗机所采用的V形尾翼布局,通过求解N-S方程的数值计算方法,得到了上反与下反V形尾翼气动布局的纵向力矩值。对比分析结果表明,上反V形尾翼由于受翼身组合体产生的下洗和速度阻滞作用,随着迎角的增加力矩曲线有上翘现象,但随着马赫数的增加而减弱;下反V形尾翼布局力矩曲线的线性度良好。     

基于FGN输入流的G/D/1排队模拟

传统的排队理论不适于分析高速网络表现出的自相似流量.通过实验仿真,主要考察平均等待时间和在队列分别为无限和有限情形下的队列尾部特征等参数,并对以FGN为输入流的G/D/1排队模型作了定性分析.结果表明在输入流的强度和方差基本相等且系统利用律大于某一阈值的情况下,队列平均等待时间随Hurst参数增大而显著增长.同时指出在相同的条件下考察队列尾部特征,具有有限队列长度的G/D/1排队模拟结果要远优于无限队列长度下的理论分析结果.      

仿生机器鱼尾鳍拍动的控制算法

两关节尾鳍拍动控制是一个在高速、大载荷下的运动控制问题,它要求同时保证速度和位置波形失真都比较小.论证了尾鳍拍动推进方式与鱼体波动推进方式的一致性,根据尾鳍拍动的运动规律导出了用于拍动控制的数学模型.基于SPC-III机器鱼硬件平台,在主臂控制上,提出了根据摆角位置解算转速,并结合时间与摆角位置关系进行速度补偿的算法;在小臂控制上,提出了根据两关节摆角位置的关系及程序循环周期解算小臂目标位置的跟随算法.对高频拍动的实现进行了探讨.在试验中对尾鳍拍动的跟随性进行了验证.