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251.
针对星载相控阵天线在轨标校技术,重点研究了S频段星载相控阵天线标校方法,论证了标校站的数量及配置要求,同时分析了标校时间和标校流程,从而提出了使用1个标校站进行粗略标校,然后再使用3个标校站进行精确标校,即改进的粗略标校+精确标校的在轨标校方法。在保证标校精度的同时,使标校站天线口径从3个7m天线降低为1个7m天线和2个0.5m天线,大大降低了系统对标校站的建设要求。当相控阵天线波束合成损失大于1dB,系统可采用单站粗略标校+三站精确标校的改进算法进行天线标校;当相控阵天线波束合成损失在1dB以内,系统可省略单站粗略标校过程直接进行三站精确标校。 相似文献
252.
253.
In this paper, the common heat source model of point and linear heat source in the numerical simulation of electron beam welding (EBW) were summarized and introduced. The combined point-linear heat source model was brought forward and to simulate the welding temperature fields of EBW and predicting the weld shape. The model parameters were put forward and regulated in the combined model, which included the ratio of point heat source to linear heat source Qpr and the distribution of linear heat source Lr. Based on the combined model, the welding temperature fields of EBW were investigated. The results show that the predicted weld shapes are conformable to those of the actual, the temperature fields are reasonable and correct by simulating with combined point-linear heat source model and the typical weld shapes are gained. 相似文献
254.
基于多块结构滑移网格,采用多参考系模型（MFR）,对某六叶螺旋桨黏性流场进行了非定常数值模拟.分别建立包围螺旋桨的旋转区域和螺旋桨以外的静止区域,很好地解决了螺旋桨的相对旋转问题.计算结果与实验结果吻合良好,验证了计算方法的正确性.对前进比为0.90和0.75情况下的桨后复杂流场进行分析,得到了螺旋桨尾涡的一些静态和动态特征,螺旋桨尾涡中包含正负两层,与实验观察到的现象一致.获得了螺旋桨对桨后轴向速度分布的影响规律:螺旋桨对桨叶45%和70%半径处轴向速度增加远大于90%半径处轴向速度;随前进比减小,该区域内轴向速度继续增加,90%半径处轴向速度几乎不变. 相似文献
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256.
混沌信号的一种简单设计方法及应用 总被引：5，自引：0，他引：5
刘文波 《南京航空航天大学学报》1998,30(3):288-292
在对一类简单的能够产生混沌现象的映射过程进行统计特性分析的基础上,利用其协方差函数特点,介绍了一种自协方差函数为ｃ（ｋ）＝ｃ（０）αｋ,０＜α＜１形式的混沌信号的简单设计方法及应用,从而为有目的地产生混沌信号,利用及分析混沌信号提供了新的信号获取途径。 相似文献
257.
Yu Gao Haiqing Xu Hongqi Zhang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
By analyzing the vector magnetograms of Huairou Solar Observing Station (HSOS) taken at the line center (0.0 Å) and the line wing (−0.12 Å) of FeI λ5324.19 Å, we make an estimate of the measured errors in transversal azimuths (δ?) caused by Faraday rotation. Since many factors, such as the magnetic saturation and scattered light, can affect the measurement accuracy of the longitudinal magnetic field in the umbrae of sunspots, we limit our study in the region ∣Bz∣ < 800 G. The main mean azimuth rotations are about 4°, 6°, 7° and 9°, while ∣Bz∣ are in the ranges of 400–500 G, 500–600 G, 600–700 G and 700–800 G, respectively. Moreover, we find there is also an azimuth rotation of about 8° at the wavelength offset −0.12 Å of the line compared against a previous numerical simulation. 相似文献
258.
《中国航空学报》2022,35(8):221-235
Aimed at the problem of instability in engine control caused by vector deflection in experiment of turbofan engines with Axisymmetric Vectoring Exhaust Nozzle (AVEN), a vector deflection stability control method of aero-engine based on Linear Active Disturbance Rejection Control (LADRC) is proposed. Firstly, based on CFD numerical simulation, aerodynamic performance model of AVEN is established, and the aerodynamic load change rule of the nozzle throat area actuator during vector deflection is revealed. Subsequently, the integrated model of AVEN/turbofan engine is established by Simulink/AMESim co-simulation. Finally, the nozzle throat area control loop based on LADRC is designed. The simulation results show that the integrated model can reflect the influence of vector deflection on the stability of the control system. The accuracy comparison between the fan rotor speed and the test data during vector deflection is larger than 1%, indicating a high degree of confidence. Compared with the conventional PID control, the designed LADRC control loop reduces the speed of the low-pressure rotor during vector deflection by 70%, which effectively improves the control stability of the vector deflection. Meanwhile, the fuel flow ratechange during the vector deflection process is smaller and more economical, which provides an important reference for engineering applications. 相似文献
259.
A. Mangalam A. Prasad 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(2):738-748
We use our semi-analytic solution of the nonlinear force-free field equation to construct three-dimensional magnetic fields that are applicable to the solar corona and study their statistical properties for estimating the degree of braiding exhibited by these fields. We present a new formula for calculating the winding number and compare it with the formula for the crossing number. The comparison is shown for a toy model of two helices and for realistic cases of nonlinear force-free fields; conceptually the formulae are nearly the same but the resulting distributions calculated for a given topology can be different. We also calculate linkages, which are useful topological quantities that are independent measures of the contribution of magnetic braiding to the total free energy and relative helicity of the field. Finally, we derive new analytical bounds for the free energy and relative helicity for the field configurations in terms of the linking number. These bounds will be of utility in estimating the braided energy available for nano-flares or for eruptions. 相似文献
260.
Ying Zhang Ping-Xiang Hu Jay Gao 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
In this paper a method based on in situ measured reflectance spectra was developed for accurately mapping salt fields in the Taibei Salt Farm in Lianyungang City of East China. After radiometric correction and geometric rectification, six multispectral ETM+ bands were fused with the panchromatic band via principal components analysis (PCA). The fused data were used to map salt fields in the farm. Salt fields were mapped 91.95% correctly in comparison with ground statistics from raw multispectral bands. This accuracy level rose to 96.4% with the use of the panchromatic band (15 m resolution). However, PCA-fused data produced the highest accuracy of 98.8%. At the zone level, coarse resolution data resulted in an accuracy of 98.93% for crystallization ponds, but only 82.68% for condensation ponds. Use of the panchromatic band alone improved the accuracy for condensation ponds but decreased the accuracy for crystallization and evaporation ponds. Results derived from PCA-fused data are highly consistent with the ground statistics at a discrepancy between 0.35% for evaporation zone and 1.80% for condensation zone. It is concluded that a fine spectral resolution is important to separation of ponds of a varying salt content while a fine spatial resolution is important to their mapped area. Ponds of a lower salt content can be mapped more accurately from fused data than from raw spectral bands. 相似文献