工艺参数对频率选择表面传输特性试验研究

制造加工曲面频率选择表面FSS(Frequency Selective Surface)的工艺参数不同会产生FSS中心谐振频率漂移以及传输系数降低.以有限大平板FSS试件为基础,利用矢量网络分析仪PNA 8363B组成的测试系统,研究了在相同条件下加工工艺、FSS附加导电层以及FSS表面电阻率对有限大平板FSS传输性能的影响规律.结果表明,不同加工方法使得平板FSS的中心谐振频率产生漂移,该差异可能是FSS单元边缘毛刺影响的结果,该影响对FSS在各种入射角条件下的传输损耗等性能也略有影响;导电层表面电阻率对FSS的传输系数有较大影响,方块电阻越大传输系数越低,且FSS中心谐振频率也有差异;附加导电层对FSS传输特性的影响不大.      

含不确定参数的复合材料板振动的 区间分析法

提出了求解具有不确定参数的复合材料板的振动固有频率区间分析法.区间分析法利用区间数学和泰勒定理,把不确定变量简化为区间向量.这样可以在较少的结构信息的情况下确定结构响应的变化区间.在样本比较小,概率统计特性缺乏,从而通常的概率统计方法不能有效应用时,区间分析仍然有效. 对复合材料板的振动固有频率的区间法公式进行了推导,并用2个数值例子与凸模型方法的解进行比较.结果表明区间分析法比凸模型方法的解区间小.      

基于特征造型技术的涡轮叶片参数化设计

针对航空发动机涡轮气冷叶片的结构特点,提出了叶片参数化建模的特征分类形式.然后,利用特征造型技术开发涡轮叶片的参数化设计系统;并以直背涡轮叶片为具体实例阐述了该参数化模块的开发过程,为航空发动机典型结构件的参数化奠定了基础.      

黏附激励下空间目标惯性参数的辨识方法

针对黏附卫星会自然激励目标改变运动状态的现象，提出一种利用黏附激励进行空间非合作目标惯性参数的辨识方法。黏附前，利用主星对目标特征点的视觉测量，建立估计目标惯性参数与相对运动参数的滤波器，并估计目标的转动惯量比和质心；黏附后，主星直接利用该滤波器估计目标的新的质心速度，并基于动量守恒原理计算目标质量。该方法不仅充分利用黏附过程的自然激励，无需常规辨识必须的主动激励，而且激励前后算法一致，无需切换。数字仿真证实了算法的有效性。     

Development of one-minute rain-rate and rain-attenuation contour maps for satellite propagation system planning in a subtropical country: South Africa

Millimeter and microwave system design at higher frequencies require as input a 1-min rain-rate cumulative distribution function for estimating the level of degradation that can be encountered at such frequency bands. Owing to the lack of 1-min rain-rate data in South Africa and the availability of 5-min and hourly rainfall data, we have used rain-rate conversion models and the refined Moupfouma model to convert the available data into 1-min rain-rate statistics. The attenuation caused by these rain rates was predicted using the International Telecommunication Union (ITU) recommendations model. The Kriging interpolation method was used to draw contour maps over different percentages of time for spatial interpolation of rain-rate values into a regular grid in order to obtain a highly consistent and predictable inter-gauge rain-rate variation over South Africa. The present results will be useful for system designers of modern broadband wireless access (BWA) and high-density cell-based Ku/Ka, Q/V band satellite systems, over the desired area of coverage in order to determine the appropriate effective isotropically radiated power (EIRP) and receiver characteristics of this region.     

充气机翼保形设计与气动特性分析

充气机翼是一种典型的柔性充气结构,涉及到变形无人机前沿技术,未来可应用于折叠飞机、科学实验研究飞机、探测火星等其他行星的飞行器。依据内切圆逼近翼型方法,通过静力学进行保形证明,以NACA0018为原型翼型,设计不同内切圆数目逼近的充气机翼,利用CFD方法对所设计的充气机翼进行气动特性分析,研究不同充气机翼的气动特性和优劣性,初步掌握内切圆逼近翼型保形方法的基本性质。最后进行充气机翼的样机制作,并通过飞行试验演示验证充气机翼的飞行性能。结果表明:在低速飞行条件下,充气机翼升力系数较标准翼型有所损失,并且随内切圆数目变化不明显,基本达到标准翼型的80%左右,阻力系数变化较为明显,几乎比标准翼型增加了1.0~1.5倍。     

Modeling and analysis of Earth’s gravity field measurement performance by inner-formation flying system

The Earth’s gravity field can be measured with high precision by constructing the purely gravitational orbit of the inner-satellite in Inner-formation Flying System (IFS), which is independently proposed by Chinese scholars and offers a new way to carry out gravity field measurement by satellite without accelerometers. In IFS, for the purpose of quickly evaluating the highest degree of recovered gravity field model and geoid error as well as analyzing the influence of system parameters on gravity field measurement, an analytical formula was established by spectral analysis method. The formula can reflect the analytical relationship between gravity field measurement performance and system parameters such as orbit altitude, the inner-satellite orbit determination error, the inner-satellite residual disturbances, data sampling interval and total measurement time. This analytical formula was then corrected by four factors introduced from numerical simulation of IFS gravity field measurement. By comparing computation results from corrected analytical formula and the actual gravity field measurement performance by CHAMP, the correctness and rationality of this analytical formula were verified. Based on this analytical formula, the influences of system parameters on IFS gravity field measurement were analyzed. It is known that gravity field measurement performance is a monotone decreasing function of orbit altitude, the inner-satellite orbit determination error, the inner-satellite residual disturbances, data sampling interval and the reciprocal of total measurement time. There is a match relationship between the inner-satellite orbit determination error and residual disturbances, in other words, the change rate of gravity field measurement performance with one of them is seriously restricted by their relative size. The analytical formula can be used to quantitatively evaluate gravity field measurement performance fast and design IFS parameters optimally. It is noted that the analytical formula and corresponding conclusions are applied to any gravity satellite which measures gravity field by satellite perturbation orbit.     

一种遥测缓变参数自动判读的新方法

针对遥测参数中缓变参数的自动判读问题，提出一种基于历史数据统计特性的遥测缓变参数自动判读新方法。首先，设计了一种以参数目标数据时标为基准的时间间隔递推算法和线性插值方法，使历史数据与目标数据的时标得到有效统一。其次，基于方向和距离函数构造了双因子等价权函数，并利用抗差最小二乘估计算法得到了参数的估值和标准差。最后，根据参数的估值和标准差对目标数据进行统计分析，依据目标数据的概率分布判断参数是否存在异常，进而实现参数的自动判读。仿真校验结果表明，该方法能有效辨识缓变参数中的异常参数，且具有较强的抑制随机噪声和抗差自适应能力。与传统以人工为主的判读方式相比，该方法能有效提高遥测参数判读的效率和准确性。     

Solar terrestrial effects of two distinct types

The occurrence frequencies or fluxes of most of the solar phenomena show a 11-year cycle like that of sunspots. However, the average characteristics of these phenomena may not show a 11-year cycle. Among the terrestrial parameters, some related directly to the occurrence frequencies of solar phenomena (for example, ionospheric number densities related to solar EUV fluxes which show 11-year cycle like sunspots) show 11-year cycles, including the double-peak structures near sunspot maxima. Other terrestrial parameters related to average characteristics may not show 11-year sunspot cycles. For example, long-term geomagnetic activity (Ap or Dst indices) is related to the average interplanetary solar wind speed V and the total magnetic field B. The average values of V depend not on the occurrence frequency of ICMEs and/or CIRs as such, but on the relative proportion of slow and high-speed events in them. Hence, V values (and Ap values) in any year could be low, normal or high irrespective of the phase of the 11-year cycle, except that during sunspot minimum, V (and Ap) values are also low. However, 2–3 years after the solar minimum (well before sunspot maximum), V values increase, oscillate near a high level for several years, and may even increase further during the declining phase of sunspot activity, due to increased influence of high-speed CIRs (corotating interplanetary regions). Thus, Ap would have no fixed relationship with sunspot activity. If some terrestrial parameter shows a 11-year cycle, chances are that the solar connection is through the occurrence frequencies (and not average characteristics) of some solar parameter.     

Comparison of calculation models for determination of the mesopause temperature using SATI images

The Spectral Airglow Temperature Imager is an instrument for ground-based spectroscopic measurements of the night-glow atmosphere emissions. This instrument was developed specially for gravity wave investigation. The measured airglow spectra are matched to synthetic spectra calculated in advance for determination of the temperature in the mesopause region where the radiation maximum of some О₂ emissions is situated. The synthetic spectra are transformed into a format which corresponds to the measured spectra in order to be matched. This transformation is based on the known values of the refractive index and the central wavelength of the interference filter used. A substantial part of the processing algorithms of the SATI images is connected with determination of these two filter parameters. The results of the original and newly-proposed algorithms for filter parameter calculation and their importance for the final results for temperature determination on the basis of the О₂ (864–868 nm) emission measurements are presented.