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本文首先介绍了合成孔径聚焦超声成像的基本原理。针对提高成像的分辨率和信噪比问题,研究了原始采样信号的相关性,提出了一种基于信号相关度加权的合成新算法和原始数据预处理方法。利用改进方法对试样进行了断面成像实验,实验结果表明:与传统的延时一叠加合成孔径算法相比,新方法提高了图像的横向分辨率和信噪比,改善了图像质量。 相似文献
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磁等离子体推力器以其推力大、比冲高等特点,成为未来深空探测、星际航行任务首选的电推力器类型,研究推力器内部等离子体流场特性,有利于解释推力器出现的物理现象。针对特定自身场磁等离子体推力器,建立磁流体模型,使用TVD Lax-Friedrich格式以及ADI方法对推力器内部及羽流进行数值求解,得到等离子体流场及等离子体参数分布情况,仿真结果显示在高电流工况下,等离子体羽流更加集中,轴向加速效果更加显著,但高电流模式下阴极温度较高,不利于阴极的使用寿命。 相似文献
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Qile Zhao Jing Guo Zhigang Hu Chuang Shi Jingnan Liu Hua Cai Xianglin Liu 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The GRACE (Gravity Recovery And Climate Experiment) monthly gravity models have been independently produced and published by several research institutions, such as Center for Space Research (CSR), GeoForschungsZentrum (GFZ), Jet Propulsion Laboratory (JPL), Centre National d’Etudes Spatiales (CNES) and Delft Institute of Earth Observation and Space Systems (DEOS). According to their processing standards, above institutions use the traditional variational approach except that the DEOS exploits the acceleration approach. The background force models employed are rather similar. The produced gravity field models generally agree with one another in the spatial pattern. However, there are some discrepancies in the gravity signal amplitude between solutions produced by different institutions. In particular, 10%–30% signal amplitude differences in some river basins can be observed. In this paper, we implemented a variant of the traditional variational approach and computed two sets of monthly gravity field solutions using the data from January 2005 to December 2006. The input data are K-band range-rates (KBRR) and kinematic orbits of GRACE satellites. The main difference in the production of our two types of models is how to deal with nuisance parameters. This type of parameters is necessary to absorb low-frequency errors in the data, which are mainly the aliasing and instrument errors. One way is to remove the nuisance parameters before estimating the geopotential coefficients, called NPARB approach in the paper. The other way is to estimate the nuisance parameters and geopotential coefficients simultaneously, called NPESS approach. These two types of solutions mainly differ in geopotential coefficients from degree 2 to 5. This can be explained by the fact that the nuisance parameters and the gravity field coefficients are highly correlated, particularly at low degrees. We compare these solutions with the official and published ones by means of spectral analysis. It is found that our solutions are, in general, consistent with others in the spatial pattern. The water storage variations of the Amazon, Chari and Ganges river basins have also been computed. The variations computed with the NPARB approach are closer to those produced by JPL and DEOS solutions, while the variations produced with the NPESS approach are in good agreement with those produced by the CSR and GFZ solutions. A simulation study is implemented with considering realistic noise and low-frequency error. The two approaches are used to recover the true model. The NPESS solution appears closer to the true one. Therefore we are inclined to estimate the nuisance parameters simultaneously with the geopential coefficients. 相似文献
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介绍了一种宽频带带状线魔T的设计原理,并采用了一种新颖的设计方法,即利用Ansoft公司的电磁场高频结构仿真软件HFSS对所设计的器件进行分析。所设计的魔T带宽可达一个倍频程以上,在设计频段(1GHz~2GHz)内,移相偏差Δ<±5°,幅度不平衡ΔA<1dB,回波损耗小于-19dB,端口隔离度小于-20dB。 相似文献