飞机俯仰角位移控制系统积分式控制规律的改进及仿真

为使飞机以足够高的准确度保持在预定飞行轨迹上,飞机俯仰角位移(9)的控制性能及稳态精度至关重要.为改进飞机俯仰角位移控制系统的控制性能,运用根轨迹法对飞机俯仰角位移控制系统的积分式控制规律进行了分析和设计,为提高(9)的稳态精度,基于SISO Design Tool设计工具,对俯仰角位移控制系统的零极点进行校正配置,实...     

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...     

飞行器管理系统需求

飞行器管理系统(VMS)将飞行、推进控制与相关的公管系统综合.飞行器管理系统的概念为性能改善带来了巨大的好处,同时对可靠性、维修性和保障性有重大改善.未来高性能的飞机将具有多操纵面/效应器以保证机动性,利用飞行/推进综合控制实现性能收益.随着更多系统的参与,综合设计的难度会增加.为确保VMS的实际应用,需要明确其计算和...     

在轨服务的相对运动耦合动力学建模与分析

研究在轨服务航天器逼近与捕获目标航天器的相对轨道姿态耦合动力学建模问题。考虑航天器姿态与对接位置的运动耦合,建立目标运行在任意轨道下的相对轨道姿态耦合动力学模型,并对模型中的运动耦合进行深入分析。设计一种非线性的输出反馈姿态控制律,将建立耦合动力学模型与CW方程进行仿真比较,验证轨道与姿态的运动耦合对两航天器对接点之间相对位置的运动影响。     

基于单目视觉的三点测量滚转角方法

确定轴对称物体的滚转角是光学测量的重要内容,具有十分广泛的工程应用背景。本文提出一种单像机测量滚转角的新方法,通过3个控制点即可完全确定物体滚转角。仿真数据计算证明了该方法的正确性和可行性。     

SNMP协议在测控网远程监控中的应用研究

简要介绍了SNMP（简单网络管理协议）管理模型,基于测控设备C/S（客户/服务器）监控模式现状,分析了测控设备监控信息传输的特点,对现有监控信息传输协议与SNMP协议进行了研究,从传输可靠性、传输效率与协议操作应用等方面进行了比较,并开展了基于SNMP协议的远程监控信息传输试验。试验结果表明,基于SNMP协议可实现测控设备参数与状态监视信息的传输。     

系留气球系统三拉索收放状态建模与仿真

系留气球是一种依靠气囊内的浮升气体获得浮力,并用缆索拴系固定的浮空器。系留气球、三根机械拉索、地面转动梁等构成系留气球三拉索收放系统,综合考虑收放系统中三拉索的运动特性,采用Matlab/Sim-ulink工具对近地三拉索收放运动进行系统建模,建立了整体的三拉索收放运动状态的仿真模型,仿真结果表明：仿真计算结果与实际飞...     

航空专用测试设备校准问题的研究

简要介绍了航空专用测试设备的概念,在计量、校准中遇到的问题以及解决问题的途径。     

Inversion of satellite gradiometry data using statistically modified integral formulas for local gravity field recovery

The satellite gravity gradiometric data can be used directly to recover the gravity anomaly at sea level using inversion of integral formulas. This approach suffers by the spatial truncation errors of the integrals, but these errors can be reduced by modifying the formulas. It allows us to consider smaller coverage of the satellite data over the region of recovery. In this study, we consider the second-order radial derivative (SORD) of disturbing potential (T_rr) and determine the gravity anomaly with a resolution of 1° × 1° at sea level by inverting the statistically modified version of SORD of extended Stokes’ formula. Also we investigate the effect of the spatial truncation error on the quality of inversion considering noise of T_rr. The numerical investigations show satisfactory results when the area of T_rr coverage is the same with that of the gravity anomaly and the integral formula is modified by the biased least-squares modification. The error of recovery will be about 6 mGal after removing the regularization bias in the presence of 1 mE noise in T_rr measured on the orbit.     

Characteristics of field line resonance type geomagnetic pulsations and variations of plasmaspheric plasma density distribution

The period of field line resonance (FLR) type geomagnetic pulsations depends on the length of the field line and on the plasma density in the inner magnetosphere (plasmasphere), where field lines are closed. Here as FLR period, the period belonging to the maximum occurrence frequency of the occurrence frequency spectrum (equivalent resonance curve) of pulsations has been considered. The resonance system may be replaced by an equivalent resonant circuit. The plasma density would correspond to the ohmic load. The plasma in the plasmasphere originates from the ionosphere, thus FLR period, occurrence frequency are also affected by the maximum electron density in the ionosphere. The FLR period has shown an enhancement with increasing F region electron density, while the occurrence frequency indicated diminishing trend (possible damping effect). Thus, the increased plasma density may be the cause of the decreased occurrence of FLR type pulsations in the winter months of solar activity maximum years (winter anomaly).