A Day and Night Separation Alternative Calibration Method for High Resolution Satellite Wide Field Imager
A technology for high-resolution satellites and imagers, applied to instruments, re-radiation of electromagnetic waves, utilization of re-radiation, etc., can solve the lack of on-board real-time dark noise signal monitoring functions, absolute radiation calibration method usage conditions, calculation processes and models Accuracy and other problems, to achieve the effect of taking into account system performance and algorithm feasibility, improving accuracy, and strong 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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