Feature Scalar Field Grid-Guided Optical-Flow Image Matching for Multi-View Images of Asteroid

Author:

Zhang Sheng1ORCID,Xue Yong12,Tang Yubing3,Zhu Ruishuan4,Jiang Xingxing1ORCID,Niu Chong1,Yin Wenping1

Affiliation:

1. School of Environment and Spatial Informatics, China University of Mining and Technology, Xuzhou 221116, China

2. School of Computing and Mathematics, College of Science and Engineering, University of Derby, Derby DE22 1GB, UK

3. Shandong Province Institute of Land Surveying and Mapping, Jinan 250013, China

4. Shandong Zhengyuan Aerial Remote Sensing Technology Co., Ltd., Jinan 250101, China

Abstract

Images captured by deep space probes exhibit large-scale variations, irregular overlap, and remarkable differences in field of view. These issues present considerable challenges for the registration of multi-view asteroid sensor images. To obtain accurate, dense, and reliable matching results of homonymous points in asteroid images, this paper proposes a new scale-invariant feature matching and displacement scalar field-guided optical-flow-tracking method. The method initially uses scale-invariant feature matching to obtain the geometric correspondence between two images. Subsequently, scalar fields of coordinate differences in the x and y directions are constructed based on this correspondence. Next, interim images are generated using the scalar field grid. Finally, optical-flow tracking is performed based on these interim images. Additionally, to ensure the reliability of the matching results, this paper introduces three methods for eliminating mismatched points: bidirectional optical-flow tracking, vector field consensus, and epipolar geometry constraints. Experimental results demonstrate that the proposed method achieves a 98% matching correctness rate and a root mean square error of 0.25 pixels. By combining the advantages of feature matching and optical-flow field methods, this approach achieves image homonymous point matching results with precision and density. The matching method exhibits robustness and strong applicability for asteroid images with cross-scale, large displacement, and large rotation angles.

Funder

National Natural Science Foundation of China

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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