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An integration time adaptive control method for atmospheric composition detection of occultation

机译:掩星大气成分探测的积分时间自适应控制方法

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When sun is used as the light source for atmospheric composition detection, it is necessary to image sun for accurate identification and stable tracking. In the course of 180 second of the occultation, the magnitude of sun light intensity through the atmosphere changes greatly. It is nearly 1100 times illumination change between the maximum atmospheric and the minimum atmospheric. And the process of light change is so severe that 2.9 times per second of light change can be reached. Therefore, it is difficult to control the integration time of sun image camera. In this paper, a novel adaptive integration time control method for occultation is presented. In this method, with the distribution of gray value in the image as the reference variable, and the concepts of speed integral PID control, the integration time adaptive control problem of high frequency imaging. The large dynamic range integration time automatic control in the occultation can be achieved.
机译:当使用太阳作为大气成分检测的光源时,必须对太阳成像以进行准确识别和稳定跟踪。在遮掩的180秒过程中,通过大气的太阳光强度的大小发生了很大变化。这是最大大气和最小大气之间的照度变化的近1100倍。而且光变的过程非常严重,每秒可达到2.9次光变。因此,难以控制太阳摄像机的积分时间。本文提出了一种新的掩星自适应积分时间控制方法。该方法以图像中灰度值的分布作为参考变量,结合速度积分PID控制的概念,解决了高频成像的积分时间自适应控制问题。可以实现掩星的大动态范围积分时间自动控制。

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