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哈尔滨工业大学航天学院空间光学工程研究中心2. 哈工大空间光学工程中心3. 哈尔滨工业大学空间光学工程研究中心
收稿日期:2008-12-22,
修回日期:2009-03-11,
网络出版日期:2009-12-25,
纸质出版日期:2009-12-25
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李克新,丛明煜,张伟. 基于STK的深空背景点目标红外序列图像生成方法[J]. 光学精密工程, 2009,17(12):3062-3068
Method of IR sequence image generation for point target in deep space based on STK[J]. Optics and precision engineering, 2009, 17(12): 3062-3068.
针对空间目标天基探测仿真系统需求,提出了一种基于STK+MATLAB 的深空背景点目标红外序列图像生成方法。点目标表面温度计算采用了比以往节点网络法计算更高效的等温简化模型以提高仿真效率;深空背景模型采用了比以往LRS(低分辨率光谱仪)模型更完备的MSX(中段空间实验卫星)红外星表的建模方法,扩展了探测系统仿真应用领域;建立了以电子数表征的目标背景照度和图像灰度转换模型。图像仿真过程中加入了卫星扰动误差、相机测量误差和焦面电子学噪声,仿真生成的图像序列更接近真实物理过程。该仿真方法可以模拟任意时刻,任意指向和任意光学视场的4-26μm的点目标红外图像序列,图像生成实时性好,仿真结果更接近真实物理过程。文章最后给出了某空间目标的红外序列图像仿真实例。
To acquire and real time process Space target information for Space-based detection systems is a challenging problem. The simulation for space-based detection systems are much more concerned in recently years. Dynamic IR image sequences generation of space target is one of the key technology. In the previous method
target temperature model is calculated by node network technique
it is high precision but consume computation
which is not necessary for point target image generation. Because the space target is very long distance from the satellite-based sensors
and the size of target is much smaller than the sensor's spatial resolution. Otherwise
the kinetic error of vehicles
the measuring error of sensors and electronic noise of PFA are not concluded in them. So
the generated images by using the previous method could not assure the validity of the simulation for space-based detection systems. In this paper
A new simulation method of IR sequence image generation for point target in deep space background based on STK and MATLAB is presented. A simple isothermal model is used to calculate the temperature of the space targets
and A model of celestial background based on MSX (Midcourse Space Experiment) IR stellar catalog is presented
Conversion model between the Irradiance of target/background and the image gray is established by calculating the electron numbers that received by the detectors. Disturbance error of satellite
measuring error of sensors and electronics noise of FPA are modeled in the simulation. it makes the generated image almost reflecting the real world. At anytime
any viewpoint and any FOV's IR sequential images from which waveband 4 to 26μm can be simulated using our method. At last of the paper
an IR image sequences of some point target are implemented. The image generation technique that presented in this paper has three merits than the previous method. The first
it is computation efficiency as the reduced target temperature model. Second
the celestial background model that presented extends the LRS stellar catalog included 5425 to the MSX stellar catalog of 177886
and the smaller FOV of sensor can be simulated. which extends the field of application of the simulation for space-based system. the third
the more complete model than previous methods is presented
included the Disturbance error of satellite
measuring error of sensors and electronics noise of FPA. and the simulated images can almost reflect the real world.
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