Day and night separation vicarious calibration method for high-definition satellite wide-view filed imager
A technology for high-resolution satellites and imagers, which is applied to instruments, electromagnetic wave re-radiation, and utilization of re-radiation, etc. It can solve the problem of absolute radiation calibration method using conditions, calculation process and model accuracy, and the lack of real-time dark noise signals on the satellite. Monitoring functions and other issues to achieve the effect of taking into account system performance and algorithm feasibility, improving accuracy, and enhancing practicability
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[0028] Below in conjunction with accompanying drawing, the present invention is described in detail, as figure 1 As shown, the specific steps are as follows:
[0029] (1) Calculation of its own dark noise offset: read the original remote sensing image data of the high-resolution satellite wide-field imager’s nighttime ocean scene, preprocess the original data, obtain the corresponding first-level remote sensing image data, and The count value of each probe in the image is calculated according to the formula ① to calculate the dark noise offset of each band of the imager;
[0030] offset λ i = Σ j = 0 n DN night , λ 1 ...
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