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131.
132.
《中国航空学报》2021,34(2):252-264
The technique of imaging a target with a complicated motion using an Inverse Synthetic Aperture Radar (ISAR) system is an effective tool in the field of radar signal processing. After the translational compensation, the received signal reflected from the target can take the form of a multi-component Polynomial Phase Signal (m-PPS), and the high quality ISAR image can be provided via the combination between the estimated parameters of the m-PPS and the Range Instantaneous-Doppler technique (RID). For a target with a high maneuvrability, the occurrence of scatterers Migration Through Resolution Cell (MTRC), caused by the rotational movement could be appearing. That is why the variation in the amplitude of the echo during the time of observation cannot be neglected. The purpose of this study is the parameters estimation of the m-PPS signal with order three in the case of the Time Varying Amplitude (TVA). The Improved-version of the Product High-order Ambiguity Function (IPHAF) with TVA is proposed to improve the quality of the ISAR image compared with traditional techniques based on a constant amplitude; the experimental outcomes confirm that the new IPHAF-TVA method presented in this study is an effective technique to make the ISAR image very clear. 相似文献
133.
压缩传感突破了 Nyquist-Shannon 采样定理的限制,从随机观测的少量测量值中即可高精度地获取图像,给成像设备的设计带来了巨大变革。压缩传感理论证明可以通过重构恢复获得比焦平面阵列分辨率更高的场景图像。尽管在理论上存在巨大优越性,压缩传感成像系统的物理实现需要考虑一些实际问题。文章围绕压缩传感成像设备进行了研究,提出了一种物理可实现的压缩成像方法,该方法利用双通道观测架构实现压缩成像中的双极性观测,解决了压缩成像理论与实际物理约束不一致的问题。采用多路技术和多膜技术实现大视场观测与多次视场观测,该方法可以单次曝光获取充足的观测值来高精度重构原图像。压缩光谱成像数值仿真实验验证了该方法的有效性和鲁棒性。 相似文献
134.
十亿像素相机可以获取信息量较大的图像,在天文观测、航空航天遥感等领域具有广泛的应用前景。受探测器和光学设计水平的限制,传统的大视场十亿像素成像通过小视场相机扫描和图像拼接实现。为解决传统十亿像素相机实时性不高的问题,文章研究一种新型多尺度大视场十亿像素成像技术,从实现十亿像素成像的条件出发,阐述该技术的原理、优势及应用领域;分析系统独特的技术指标,包括物理锥角、重叠率等,梳理和归纳新型多尺度大视场十亿像素成像系统走向实用化过程中必须克服的关键技术。研究结果表明,该技术可在不提高系统复杂性的情况下大幅提高监视实时性。 相似文献
135.
空间机械臂辅助舱段对接过程中存在测量与控制误差,易导致对接机构间存在较大接触力,传统FMA (Force MomentAccommodation)控制方法在测量接触力时无法消除大负载惯性力对测量的影响,且测量仪器的引入会进一步降低空间柔性机械臂的刚度。为此,文章提出了柔性机械臂辅助大负载空间舱段对接的阻抗控制方法,采用拉格朗日法推导了空间机械臂的关节输入力矩方程作为前馈输入,建立了含动力学前馈的空间机械臂阻抗控制程序,并以在商业软件ADAMS中建立的空间柔性机械臂与对接舱段组成的系统动力学模型作为控制对象,对系统进行ADAMS灢Matlab联合仿真。仿真结果表明,按照此控制方法,系统可克服外力干扰使目标解析点按照期望的方式运动;同时,通过测量机械臂关节运动参数即可实现对外力的准确感知,而不需额外添加力传感器,既消除了大负载惯性力对测量的影响,也不会导致柔性机械臂刚度的降低。 相似文献
136.
Mourad Lazri Soltane Ameur Yacine Mohia 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
In the present paper, an artificial neural network (ANN) based technique has been developed to estimate instantaneous rainfall by using brightness temperature from the IR sensors of SEVIRI radiometer, onboard Meteosat Second Generation (MSG) satellite. The study is carried out over north of Algeria. For estimation of rainfall, weight matrices of two ANNs namely MLP1 and MLP2 are developed. MLP1 is to identify raining or non-raining pixels. When rainy pixels are identified, then for those pixels, instantaneous rainfall is estimated by using MLP2. For identification of raining and non raining pixels, 7 input parameters from the IR sensors are utilized. Corresponding data of raining/non-raining pixels are taken from radar. For instantaneous rainfall estimation, 14 input parameters are utilized, where 7 parameters are information about raining pixels and 7 parameters are related with cloud features. The results obtained show the neural network performs reasonably well. 相似文献
137.
Sriram Saran Anup DasShiv Mohan Manab Chakraborty 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2014
The surface layer of the Moon preserves vital evidences of lunar impact and cratering processes due to the absence of any Aeolian and fluvial erosion processes acting on it. By examining these evidences, which are recorded throughout the evolutionary history of the Moon, several basic aspects of lunar science can be understood, and this has direct relevance to the surfaces of other airless bodies within the solar system. In this study, rock abundance data obtained from Thermal Infrared (TIR) observations and radar Circular Polarization Ratio (CPR) data sets obtained from polarimetric SAR observations were correlated at some sample sites on the lunar surface. Preliminary results yielded qualitative and quantitative estimates for surface rock abundances. Except at distal ejecta deposits of young, bright craters a general correlation was observed between the two datasets. Mixed results were observed from the impact melt flows where the situation is complex due to the possible subsurface-volume and volume-subsurface interactions of the radar waves. But the flow features were clearly separated from the interior and ejecta regions of their parent craters in terms of CPR and rock abundances. The extent and distributions of pyroclastic deposits and dark haloed regions could not be distinctly identified at the resolution of datasets utilized. Near Gerasimovich D crater, the Diviner Radiometer has provided the first TIR observations of a newly discovered impact melt flow which was not visible in the optical imagery. This facilitated the first ever quantitative comparisons of the radar CPR and rock abundance values near such a region. Also, significant differences in spatial patterns between the radar and rock concentration data sets were observed, owing to the differences in the sensitivity of the two observations. 相似文献
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