一种非线性部分极曲线的试飞方法

介绍了一种不测推力获取非线性部分极曲线的试飞方法。从飞机纵向动力学方程出发,推导出了利用试飞数据计算非线性部分诱导阻力系数Ａ值的公式,在铅垂对称平面内进行了飞行试验。试验结果表明：不测推力法试飞结果同测推力法试飞结果、风洞预测值以及Ｊ７原型机资料值具有良好的一致性,不测推力法是一种经济、可靠、简便而有效的试飞方法,可用于同类型飞机的非线性曲线试飞研究。     

SH波对结构表面上含有多个半圆形介质夹杂的散射

利用复变函数和多极坐标系的方法,研究了在结构表面上含有多个半圆形介质夹杂的散射问题,首先给出 SH波对多个半圆形介质夹杂的散射波函数,并利用多极坐标系的方法,来满足介质界面上的连续条件和表面上的边界条件,归结为对一组无穷代数方程组的求解,简化了问题的求解。作为算例,对结构水平面上含有 2个半圆形夹杂介质进行分析,并讨论了夹杂介质参数的变化及孔距对位移的影响。     

极地科考小型无人飞行器

针对小型无人飞行器在极地科考中的抗风扰动问题,通过神经网络改进卡尔曼滤波算法,提高小型无人飞行器对环境的适应性.基于小型无人飞行器自身状态信息与误差信息,在线调整系统的量测噪声和估计参数,提高信息融合精度;利用矢量域方法构建轨迹跟踪控制算法,基于目标航迹在线调整航向,提高小型无人飞行器在顺风、逆风、转弯的飞行品质和压航线精度.经过大量的仿真试验、实际飞行试验验证了方法的有效性,改进的卡尔曼滤波算法可以提供长时高精度信息,小型无人飞行器可以在野外6级风源扰动的情况下,实现稳定飞行,平均误差不超过10m.小型无人飞行器在南极实地科考中得到成功应用.     

修正极坐标系下雷达与ESM航迹对准关联

研究了存在系统误差时修正极坐标系(MPC)下的雷达与电子支援措施(ESM)航迹关联问题。系统误差导致MPC下雷达和ESM的角度估计产生偏移,而对角度变化率、距变率与距离的比值(ITG)的估计影响不大;结合非中心卡方分布的知识,分析了雷达与ESM的测量误差对非中心参数和正确关联概率的影响;提出了一种基于积分重合度的雷达与ESM航迹对准关联算法。首先将雷达与ESM的目标映射到角度-角度变化率空间,分别得到了雷达与ESM的目标曲线,然后对两目标曲线求积分重合度,估计出雷达与ESM测角系统误差的偏移量,对偏移量补偿后进行雷达与ESM的航迹关联。仿真结果表明,本文所提算法能有效地提高存在系统误差时雷达与ESM正确航迹关联概率。     

Sawtooth substorms generated under conditions of the steadily high solar wind energy input into the magnetosphere: Relationship between PC, AL and ASYM indices

Periodicity in occurrence of magnetic disturbances in polar cap and auroral zone under conditions of steady and powerful solar wind influence on the magnetosphere is analyzed on the example of 9 storm events with distinctly expressed sawtooth substorms (N = 48). Relationships between the polar cap magnetic activity (PC-index), magnetic disturbances in the auroral zone (AL-index) and value of the ring current asymmetry (ASYM index) were examined within the intervals of the PC growth phase and the PC decline phase inherent to each substorm. It is shown that the substorm sudden onsets are always preceded by the PC growth and that the substorm development does not affect the PC growth rate. On achieving the disturbance maximum, the PC and AL indices are simultaneously fall down to the level preceding the substorm, so that the higher the substorm intensity, the larger is the AL and PC drop in the decline phase. The ASYM index increases and decreases in conformity with the PC and AL behavior, the correlation between ASYM and PC being better than between ASYM and AL. Level of the solar wind energy input into the magnetosphere determines periodicity and intensity of disturbances: the higher the coupling function E_KL, the higher is substorm intensity and shorter is substorm length. Taking into account the permanently high level of auroral activity and inconsistency of aurora behavior and magnetic onsets during sawtooth substorms, the conclusion is made that auroral ionosphere conductivity is typically high and ensures an extremely high intensity of field-aligned currents in R1 FAC system. The periodicity of sawtooth substorms is determined by recurrent depletions and restorations of R1 currents, which are responsible for coordinated variations of magnetic activity in the polar cap and auroral zone.     

Imaging interplanetary CMEs at radio frequency from solar polar orbit

Coronal mass ejections (CMEs) represent a great concentration of mass and energy input into the lower corona. They have come to be recognized as the major driver of physical conditions change in the Sun–Earth system. Consequently, observations of CMEs are important for understanding and ultimately predicting space weather conditions. This paper discusses a proposed mission, the Solar Polar Orbit Radio Telescope (SPORT) mission, which will observe the propagation of interplanetary CMEs to distances of near 0.35 AU from the Sun. The orbit of SPORT is an elliptical solar polar orbit. The inclination angle between the orbit and ecliptic plane should be about 90°. The main payload on board SPORT will be an imaging radiometer working at the meter wavelength band (radio telescope), which can follow the propagation of interplanetary CMEs. The images that are obtained by the radio telescope embody the brightness temperature of the objectives. Due to the very large size required for the antenna aperture of the radio telescope, we adopt interferometric imaging technology to reduce it. Interferometric imaging technology is based on indirect spatial frequency domain measurements plus Fourier transformation. The SPORT spacecraft will also be equipped with a set of optical and in situ measurement instruments such as a EUV solar telescope, a solar wind ion instrument, an energetic particle detector, a magnetometer, a wave detector and a solar radio burst spectrometer.     

修正的跨声速小扰动方程以及与其相容的激波方程

本文给出了与修正的跨声速小扰动(MSD)方程相容的激波方程,计算证明它的极曲线与精确的激波极曲线十分接近。     

FY-1C/D极轨气象卫星10通道扫描辐射计及其在轨运行

介绍了风云一号(FY-1)C，D极轨气象卫星10通道扫描辐射计的总体构成。给出了扫描辐射计性能的在轨测试结果，概述了研制中的技术创新点。与国内外同类仪器比较的结果表明，两星扫描辐射计寿命期初和期末的性能均满足任务书要求，其主要性能指标与美国NOAA卫星相当，甚至更佳。     

FY-1C/D极轨气象卫星的运行和应用

简要介绍了风云一号(FY-1)C，D极轨气象卫星的运行情况。运行期间，在洪涝、火情、干旱和积雪等自然灾害的监测服务，沙尘暴、大雾和海冰等环境监测服务，全球资料应用，以及天气分析方面发挥了重要的作用．并可提供气象卫星数据的共享服务。两星在大范围自然灾害监测和评估等领城取得了显著的社会和经济效益，并在国内国际产生了重大影响。     

FY-3A极轨气象卫星

介绍了我国研制的风云三号A(FY-3A)极轨气象卫星的基本任务、轨道与发射窗口、构型与布局、主要技术参数、探测仪器配置、图像资料传输与存储,以及姿轨控和数管系统等总体概况.分析了卫星的技术特点.介绍了卫星入轨过程、平台和数传等在轨运行状况.给出了遥感仪器的工作及其部分应用结果.卫星近4个月的运行稳定,获取了大量的气象和环境数据.初步测试结果表明:FY-3A卫星大部分仪器性能与国际同类仪器比对一致,已达国际先进水平.