2011
DOI: 10.1117/12.900195
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A relative radiometric correction method for linear array push-broom imagery

Abstract: The linear array CCD camera is the main sensor on the push-broom satellite. Because of the difference response among the CCD detectors, the striping noise is an obvious phenomenon in the remote sensing image along the scanning direction, which can seriously affect the image quality and quantitative application. The object of relative radiometric calibration is to eliminate them.As the state of satellite electronics varies from orbit to orbit, an automatic de-striping algorithm is needed that depends only on in… Show more

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Cited by 2 publications
(2 citation statements)
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“…The data of a raw image for sensitivity compensation is B, the ramp test-object is represented as a matrix R where each row is an array's data on the same ramp thickness. The vector Z is the values proportional to d i from (7). Number of rows in R and Z is the same.…”
Section: Compensation Of Different Sensitive Elements X-ray Responsementioning
confidence: 99%
“…The data of a raw image for sensitivity compensation is B, the ramp test-object is represented as a matrix R where each row is an array's data on the same ramp thickness. The vector Z is the values proportional to d i from (7). Number of rows in R and Z is the same.…”
Section: Compensation Of Different Sensitive Elements X-ray Responsementioning
confidence: 99%
“…This method was designed to suit infrared images. Nevertheless, it can be applied to images produced by scanners, push-broom satellites [8,2] (where this problem is called relative radiometric correction or normalization), non equalized CCDs, etc.…”
Section: Introductionmentioning
confidence: 99%