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Stray Light Analysis and Baffle Design of Remote Sensing Camera for Microsatellite

机译:微卫星遥感摄像机杂散光分析与挡板设计

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A two-mirror catadioptric system with corrective lens groups is adopted in the remote sensing camera of microsatellite. Compared with the refractive system, it has the advantage that its performance is hardly influenced by thermal environment. Stray light results in image blur and the contrast reduction of the camera. It is necessary to analyze and control it. In traditional way, stray light can be effectively suppressed with a long baffle, which is not suitable for microsatellites with limited space. And a compact one with high performance is designed. First of all, model of the camera is set up and its stray light is analyzed with Lighttools. The main and the primary baffles are designed and optimized. Then the point source transmittance is calculated to evaluate and verify the designs. Its veiling glare index is also simulated and calculated based on black-patch measurement.
机译:微卫星遥感摄像机采用了具有校正镜组的双镜折反射系统。与折射系统相比,它的优点是其性能几乎不受热环境的影响。杂散光会导致图像模糊并降低相机的对比度。有必要对其进行分析和控制。以传统方式,可以用长挡板有效地抑制杂散光,这不适用于空间有限的微卫星。并设计了一种高性能的紧凑型产品。首先,设置摄像机的模型,并使用Lighttools分析其杂散光。主挡板和主挡板经过设计和优化。然后计算点源透射率,以评估和验证设计。还基于黑斑测量来模拟和计算其面纱眩光指数。

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