2021
DOI: 10.3390/s21041188
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An Infrared-Visible Image Registration Method Based on the Constrained Point Feature

Abstract: It is difficult to find correct correspondences for infrared and visible image registration because of different imaging principles. Traditional registration methods based on the point feature require designing the complicated feature descriptor and eliminate mismatched points, which results in unsatisfactory precision and much calculation time. To tackle these problems, this paper presents an artful method based on constrained point features to align infrared and visible images. The proposed method principall… Show more

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Cited by 8 publications
(3 citation statements)
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“…Li et al [12] proposed a method for registering infrared and visible images based on constrained point features to address the high complexity of traditional point features. This approach avoids the construction of complex feature descriptors and introduces advanced semantic information to improve the registration accuracy.…”
Section: Related Workmentioning
confidence: 99%
“…Li et al [12] proposed a method for registering infrared and visible images based on constrained point features to address the high complexity of traditional point features. This approach avoids the construction of complex feature descriptors and introduces advanced semantic information to improve the registration accuracy.…”
Section: Related Workmentioning
confidence: 99%
“…It is therefore necessary to convert the collected images into the same coordinate system and calibrate feature relations between two images through remote sensing image registration, so as to carry out the application of the following steps [12]. Remote sensing image registration technology is the basis of various remote sensing applications and is key to determining the application effect [13][14][15][16].…”
Section: Introductionmentioning
confidence: 99%
“…On the one hand, if all observed star points are directly matched with all predicted star points one by one (the existing matching method that is widely used in traditional area of star trackers), the complexity and the time of the star matching step will be significantly increased, thus resulting in the star matching step becoming the new bottleneck of the MEIA’s attitude update rate. On the other hand, although the mainstream feature points-based image registration methods are quite popular and successful in many applications [ 23 , 24 , 25 ], they are not applicable for the above star matching situation. This is because the above matching methods are mainly used to solve the point matching problem between two real images (i.e., the matching image and the matched image), while the star matching step only contains one real image (i.e., the observed star image) and one dataset of the centroid information of the predicted star points.…”
Section: Introductionmentioning
confidence: 99%