Passive Aperture Synthesis Using Pulsar’s Emissions

A. Lazarov, C. Kabakchiev, C. Minchev, I. Garvanov
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Abstract

The aim of the study is imaging of moving objects, asteroids illuminated by continuous coherent wideband signals illuminated by pulsars. As pulsars are placed on hundreds of light years from the Earth, objects crossing pulsars’ emission beams are considered as second sources of electromagnetic waves, carrying object’s shape and velocity information that ca be extracted by application pulsar emission-based inverse aperture synthesis. Inverse synthetic aperture radar (ISAR) scenario, geometry and kinematics are analytically described. Models of pulsar signals and ISAR signals secondary emitted by asteroids are suggested White Gaussian noise of high level is added to the ISAR signal in order to approach scenario to reality. Two-dimensional fast Fourier transform for image extraction is applied To verify mathematical model and imaging algorithms numerical experiments are carried out.
利用脉冲星发射进行被动孔径合成
这项研究的目的是对运动物体进行成像,小行星被脉冲星发出的连续相干宽带信号照亮。由于脉冲星被放置在距离地球数百光年的地方,穿过脉冲星发射光束的物体被认为是电磁波的第二源,携带着物体的形状和速度信息,这些信息可以通过基于脉冲星发射的逆孔径合成应用来提取。对逆合成孔径雷达(ISAR)的场景、几何和运动学进行了解析描述。提出了脉冲星信号和小行星二次发射ISAR信号的模型,在ISAR信号中加入高电平高斯白噪声,使其更接近真实场景。采用二维快速傅里叶变换进行图像提取,并进行了数值实验验证数学模型和成像算法。
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