Method for eliminating tailing light lines of frame transfer type CCD (charge coupled device) sensor in star image
A frame transfer, in-image technology, applied in image communication, TV, color TV components, etc., can solve problems such as increasing the signal-to-noise ratio of weak and small targets, increasing noise points, etc.
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[0035] 1. Establish the model of the trailing bright line of the frame transfer CCD sensor.
[0036] The brightness of the stars in the field of view of the starry sky image is too high, which causes electron overflow in the entire row or column of the CCD sensor. The trailing area is usually a straight line that passes through the center of a bright star and runs through the row or column direction of the entire image. The following takes the vertical bright line as an example to illustrate the elimination method; the original image is divided into two parts, one part is the image without trailing, and the other part is the trailing bright line. i is the row coordinate of the pixel in column j, and the star light source is constant during the exposure period and transfer time. During the exposure period τ, the number of photons accumulated by pixel i is:
[0037] N' i,j =kτA i,j (1)
[0038] In the formula, A i,j is the radiation intensity on pixel i, and k is a cons...
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