多螺旋桨太阳能无人机横航向操稳特性研究

首先分析了大型高空长航时太阳能无人机由于超大展弦比和高效多螺旋桨带来的航向阻尼增量和航向操纵导数,接着分析了由此带来的横航向动态特性变化,并结合多螺旋桨的操纵特性,提出了多桨航向控制方法,最后进行了仿真验证.结果表明,分布式多桨布局对提高该类无人机的横航向稳定性有较大作用,以多桨的转速变化量最小为目标的最优化航向控制分配方法对超长航时飞行很有利.     

无人机编队构成的分散最优控制方法研究

针对无长机带领、具有固定无向通信拓扑的无人机编队构成控制问题,提出了一种基于"相邻"无人机状态反馈的分散最优控制方法。该方法采用Laplacian矩阵描述编队通信结构,以"相邻"无人机与编队构型间的相对状态误差构建分散最优控制模型,并通过求解具有LMI约束的线性目标最优化问题得到编队各无人机的分散最优控制律。该方法使得多无人机在分散协同的前提下,基于局部信息快速准确地形成预定编队构型,达到运动方向和速度的一致性。仿真实验验证了该方法的有效性。     

多无人机对地攻击任务分配算法

在不确定条件下的战场环境中,实时有效的动态任务分配是多无人机顺利完成对地攻击任务的关键.文章基于拍卖机制原理提出了多无人机的动态任务分配算法,给出了算法流程,构建了收益计算函数,并对算法效率进行了分析.仿真试验表明所提出的算法同传统方法相比,大大减少了通信计算量,具有更好的实时性     

变体无人机动力学模型及切换控制研究

针对能够在飞行过程中进行结构变形的变体无人机,考虑由变形引起的气动力与力矩,惯性力与力矩的非线性变化,建立其在质点系假设条件下的多体动力学模型。根据切换系统理论,将变体无人机视为一类线性切换系统,选择设计点,采用极点配置方法针对各设计点处的线性子系统设计控制器,再制定以变形量为决策变量的控制切换方案,构成切换控制系统。通过建立公共Lyapunov函数,推导了能够保证闭环切换系统在结构变形过程中一致有界的充分条件。以变体无人机Fire-Bee为例,验证了方案的有效性,仿真结果表明闭环系统无论在固定结构下还是变形过程中都具有良好的动态特性。     

无人机遥控驾驶关键技术研究与飞行品质分析

无人机遥控驾驶方式相对程控方式来说,在时间延迟、情景遥现、数据链性能优化以及飞行控制等方面的要求较高,而这些因素也成为了困扰无人机遥控驾驶发展和应用的关键.借鉴无人机技术验证平台地面闭环试验的结果,以时间延迟、数据链路性能为重点针对无人机遥控驾驶所面临的各种关键技术难点进行了深入的分析、研究,提出了合理的关键技术解决方...     

The Modulation of Galactic Cosmic Rays in the Heliosphere: Theory and Models

Almost all theoretical and numerical models for the modulation of cosmic ray in the heliosphere are based on Parker's transport equation which contains all the important basic physical processes. The relative importance of the various mechanisms is however not established and may vary significantly over 22 years. The simultaneous measurements of solar wind parameters, heliospheric magnetic field properties and cosmic rays over a wide range of energies and positions in the heliosphere have brought the realization that modulation is much more complicated than what the original drift models predicted. In the process the sophistication of models based on solving Parker's equation has increased by orders of magnitude. A short review of the global modulation of cosmic rays is given from a theoretical and modelling point of view.     

Energetic particles at high latitudes

We review work on diffusion coefficients of energetic particles with an attempt to extract implications on their behaviour at high latitudes. In the ecliptic plane results from solar energetic particle propagation between the Sun and about 5 AU can be described by an effective radial mean free path _r which is approximately constant as a function of distancer. When particle propagation in three dimensions in the heliosphere is considered it is not sufficient to consider _r only. Jovian electrons can be used as probes to determine the parameters of three-dimensional diffusion. In the polar regions diffusion is dominated by its parallel component. Some predictions how should vary with latitude are discussed. For different choices of this variation we present expectations for intensity-time profiles of solar particle events during the Ulysses polar passages.     

影响螺旋桨式无人机安全发射的诸因素

根据无人机的零长发射原理,通过多个型号的发射仿真计算和发射试验分析,详细探讨了影响无人机安全发射的固有参数和外部参数,总结出影响螺桨式无人机安全发射的主要因素有：单发螺旋桨的反扭矩,火箭推力线相对重心的位置,火箭安装角,机体发射角,舵机死区及发射环境等。最后,以发射安全高度、速度、过载为约束条件,给出了火箭总冲、推力线位置、火箭安装角、机体发射角、发射风向和风速等参数的确定方法,该方法对保证无人机     

Solar Irradiance Variability Since 1978

Since November 1978 a set of total solar irradiance (TSI) measurements from space is available, yielding a time series of more than 25 years. Presently, there are three TSI composites available, called PMOD, ACRIM and IRMB, which are all constructed from the same original data, but use different procedures to correct for sensitivity changes. The PMOD composite is the only one which also corrects the early HF data for degradation. The results from the detailed analysis of the VIRGO radiometry allow a good understanding of the effects influencing the long-term behaviour of classical radiometers in space. Thus, a re-analysis of the behaviour of HF/NIMBUS-7 and ACRIM-I/SMM was indicated. For the former the situation is complicated by the fact that there are no in-flight means to determine changes due to exposure to solar radiation by comparison with a less exposed radiometer on the same spacecraft. The geometry and optical property of the cavity of HF is, however, very similar to the PMO6-type radiometers, so the behaviour of the PMO6V radiometers on VIRGO can be used as a model. ACRIM-I had to be revised mainly due to a henceforth undetected early increase and a more detailed analysis of its degradation. The results are not only important for solar radiometry from space, but they also provide a more reliable TSI during cycle 21. The differences between the revised PMOD composite and the ACRIM and IRMB are discussed by comparison with a TSI reconstruction from Kitt-Peak magnetograms. As the PMOD composite is the only one which has reliable data for cycle 21, the behaviour of the three solar cycles can now be compared and the similarities and differences discussed.     

Global Response of Martian Plasma Environment to an Interplanetary Structure: From Ena and Plasma Observations at Mars

As a part of the global plasma environment study of Mars and its response to the solar wind, we have analyzed a peculiar case of the subsolar energetic neutral atom (ENA) jet observed on June 7, 2004 by the Neutral Particle Detector (NPD) on board the Mars Express satellite. The “subsolar ENA jet” is generated by the interaction between the solar wind and the Martian exosphere, and is one of the most intense sources of ENA flux observed in the vicinity of Mars. On June 7, 2004 (orbit 485 of Mars Express), the NPD observed a very intense subsolar ENA jet, which then abruptly decreased within ∼10 sec followed by quasi-periodic (∼1 min) flux variations. Simultaneously, the plasma sensors detected a solar wind structure, which was most likely an interplanetary shock surface. The abrupt decrease of the ENA flux and the quasi-periodic flux variations can be understood in the framework of the global response of the Martian plasma obstacle to the interplanetary shock. The generation region of the subsolar ENA jet was pushed towards the planet by the interplanetary shock; and therefore, Mars Express went out of the ENA jet region. Associated global vibrations of the Martian plasma obstacle may have been the cause of the quasi-periodic flux variations of the ENA flux at the spacecraft location.